Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati H$
 1999)
    Global velocity field and bubbles in the blue compact dwarf galaxy Mrk
    86.
oTable 3: <[M98b] NGC 2537-A> (Nos B, C) added. Text, Figs: <[GZG99]    NN> N=4 among (Nos 1-55).
 Auth.:GIL DE PAZ A.+

Details on Acronym:   [GZK2003]
   [GZK2003] (Gusev+Zasov+Kaisin, 2003) (Not yet in Simbad) Write:<<[GZK2003] NN>> N: 11 Object:Region  (SIMBAD class: PartofG =) Part of a Galaxy Note:Photometry of NGC 4136. N=11 regions of star formation are found. in source:NGC 4136 Ref:=2003AstL...29..363G byGUSEV A.S. , ZASOV A.V., KAISIN S.S. Astron. Lett., 29, 363-371 (2003) Photometry of the low-luminosity spiral galaxy NGC 4136. oTable 3: <[GZK2003] NN> (Nos 1-11). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [GZK2010]
   [GZK2010] (Galvan-Madrid) + Zhang + Keto+, 2010 Write:<<[GZK2010] MMN-Main>>
<<[GZK2010] MMN-WW>>
<<[GZK2010] MM1-Ridge>> N: 2+5+1 Object:(mm)  (SIMBAD class: Radio(mm) = millimetric Radio-source) Note:2010ApJ... 725...17G: SMA 1.3mm and 0.9mm continuum observations of N=5 sources in the W33A massive star formation region.
2017MNRAS.467L.120M: ALMA band 6 (230GHz) and 7 (345GHz) observations of N=3 sources in [VVE2000] W33A MM 1. in source:W 33:W 33A = W 33A Ref:=2010ApJ...725...17G byGALVAN-MADRID R. , ZHANG Q., KETO E., HO P.T.P., ZAPATA L.A., RODRIGUEZ L.F., PINEDA J.E., VAZQUEZ-SEMADENI E. Astrophys. J., 725, 17-28 (2010) From the convergence of filaments to disk-outflow accretion: massive star formation in W33A. oTable 2: <[GZK2010] MMN-Main> (Nos MM1-Main and MM2-Main), <[GZK2010] MMN-WW> (Nos MM1-NW, MM1-SE, MM2-NE). Ref:=2017MNRAS.467L.120M byM AUD L.T., HOARE M.G., GALVAN-MADRID R., ZHANG Q., DE WIT W.J., KETO E., JOHNSTON K.G., PINEDA J.E. Mon. Not. R. Astron. Soc., 467L, 120-124 (2017) The ALMA view of W33A: a spiral filament feeding the candidate disc in MM1-Main. oFig. 1, Table 1: <[GZK2010] MM1-W> (Nos E, S) added, <[GZK2010] MM1-Ridge> N=1. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [GZR2015]
   [GZR2015] 6.06.28 (Glushkova+Zabolotskikh+Rastorguev+, 2015) Write:<<[GZR2015] OSC DDD.ddddd+DD.ddddd>> N: 8 Object:Cluster of *  (SIMBAD class: Cl* = Cluster of Stars) Stat:is completely incorporated in Simbad Note:N=8 open star clusters (OSCs) identified in a search for young star clusters and associations near known Cepheids.
Use of 2MASS data. Ref:=2015BaltA..24..360G byGLUSHKOVA E.V. , ZABOLOTSKIKH M.V., RASTORGUEV A.S., GRUDSKAYA A.V. BaltA, 24, 360-366 (20 15) A search for new open clusters hosting cepheids. oTable 1, Paragr. 3: <[GZR2015] OSC DDD.ddddd+DD.ddddd> N=4+4. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [GZW2002]
   [GZW2002] (Giacconi+Zirm+Wang+, 2002)= (CDFS) Write:<<[GZW2002] Main NNN>>
<<[GZW2002] SExtractor NN>>
<<[GZW2002] WAVDETECT NN>>
<<[GZW2002] XID NNN>> N: 346+3 Object:(X)  (SIMBAD class: X = X-ray source) Note:Chandra Catalog of the CDFS.
Table 2: Main catalog, format 'Main NNN', (Nos 1-304).
Table 3: Objects observed only with SExtractor, format 'SExtractor NN', (Nos 1-28).
Table 4: Objects observed only with WAVDETECT, format 'WAVDETECT NN', (Nos 1-14).
Tables 2, 3, 4, col(2): Another format 'XID' is introduced by the authors N=304+28+14 among (Nos 1-653).
See also CXOCDFS, [SBH2004].
In 2004ApJS..155..271S, [GZW2002] XID 901, 902, 903 are added. in source:NAME CDFS Ref:=2002ApJS..139..369G byGIACCONI R. , ZIRM A., WANG J., ROSATI P., NONINO M., TOZZI P., GILLI R., MAINIERI V., HASINGER G., KEWLEY L., BERGERON J., BORGANI S., GILMOZZI R., GROGIN N. Astrophys. J., Suppl. Ser., 139, 369-410 (2002) Chandra Deep Field South: the 1 Ms catalog. oCXOCDFS J033260.0-274748 translated into CXOCDFS J033300.0-274748 oTable 2: <[GZW2002] Main NNN> (Nos 1-304) = <[GZW2002] XID NNN> N=304 = <CXOCDFS JHHMMSS.s+DDMMSS> N=304. Table 3: <[GZW2002] SExtractor NN> (Nos 1-28) = <[GZW2002] XID NNN> N=28 = <CXOCDFS JHHMMSS.s+DDMMSS> N=28. Table 4: <[GZW2002] WAVDETECT NN> (Nos 1-14) = <[GZW2002] XID NNN> N=14 = <CXOCDFS JHHMMSS.s+DDMMSS> N=14. Ref:=2004ApJS..155..271S bySZOKOLY G.P. , BERGERON J., HASINGER G., LEHMANN I., KEWLEY L., MAINIERI V., NONINO M., ROSATI P., GIACCONI R., GILLI R., GILMOZZI R., NORMAN C., ROMANIELLO M., SCHREIER E., TOZZI P., WANG J.X., ZHENG W., ZIRM A. Astrophys. J., Suppl. Ser., 155, 271-349 (2004) The Chandra Deep Field-South: Optical spectroscopy. I.. oTables 4, 8: <[SBH2004] JHHMMSS.ss+DDMMSS.s> N=288+139. Tab les 4, 8: <[SBH2004] XID NNNa> N=103+50. Table 9: <[SBH2004] NNNNN> N=124 among (Nos 12-60041). Table 5: <[GZW2002] XID NNN> (Nos 901-903) added. =E=Catalogue in electronic form as J/ApJS/139/369 =E=Catalogue in electronic form as J/ApJS/155/271 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [GZW2003]
   [GZW2003] (Georgantopoulos+Zezas+Ward, 2003) Write:<<[GZW2003] JHHMMSS.s+DDMMSS>> N: 2 Object:(X)  (SIMBAD class: X = X) -ray source Stat:is completely incorporated in Simbad Note:Chandra observations of IRAS 00317-2142.
N=2 point-source eastward of IRAS source. Ref:=2003ApJ...584..129G byGEORGANTOPOULOS I. , ZEZAS A., WARD M.J. Astrophys. J., 584, 129-134 (2003) X-Ray-Luminous galaxies. I. Chandra observations of IRAS 00317-2142. oText: <[GZW2003] JHHMMSS.s+DDMMSS> N=2. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [GZZ2000]
   [GZZ2000] (Gonzalez+Zabludoff+Zaritsky+, 2000) (Not yet in Simbad) Write:<<[GZZ2000] A>> N: 3 Object:Region  (SIMBAD class: Regio) n = Region defined in the sky Note:N=3 regions of excess brightness in ACO 1651. in source:ACO 1651 Ref:=2000ApJ...536..561G byGONZALEZ A.H. , ZABLUDOFF A.I., ZARITSKY D., DALCANTON J.J. Astrophys. J., 536, 561-570 (2000) Measuring the diffuse optical light in Abell 1651. o(Erratum) erratum vol. 611, p. 1208 (2004) oFig.6: <[GZZ2000] A> (Nos A-C). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   H
   H (Higgs) (Not yet in Simbad) ***** Avoid the usage of H, prefer Hig
Details on Acronym:   H
   H (Hubble) ***** Avoid the usage of H, prefer BASW Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (Harten) ***** Avoid the usage of H, prefer [BHJ77] Originof the Acronym: L (1980A&A....90..246I)
Details on Acronym:   H
   H (HDF) ***** Avoid the usage of H, prefer [CSS2000] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   H
   H (HI Hole) ***** Avoid the usage of H, prefer [DD90] Originof the Acronym: L (2001PASJ...53..663O)
Details on Acronym:   H
   H (Hyland+) ***** Avoid the usage of H, prefer Dor Originof the Acronym: L (1998A&A...331..857J)
Details on Acronym:   H
   H (HEAO satellite)= (HEAO) Write:<<H HHMM+DD>>
<<H HHMM+DDd>> N: 60+114 Object:(X)  (SIMBAD class: X = X-ray source) Note:1979ApJS...40..657M: N=60, 47 are new sources, All sky, Energy 3-17 keV. 1983ApJS...51....1N: N=114, 54 were previously undiscovered and 32 remain unidentified. The catalogue contains a listing of all counterpart identif. and a cross-reference to all HEAO 1 A-2 low energy detector team publications on the catalogue sources complete through the end of 1981. Ref:=1979ApJS...40..657M byMARSHALL F.E. , BOLDT E.A., HOLT S.S., MUSHOTZKY R.F., PRAVDO S.H., ROTHSCHILD R.E., SERLEMITSOS P.J. Astrophys. J., Suppl. Ser., 40, 657-666 (1979) New hard X-ray sources observed with HEAO A-2. oTable 2: <H HHMM+DDd> N=47 Ref:=1983ApJS...51....1N byNUGENT J.J. , JENSEN K.A., NOUSEK J.A., GARMIRE G.P., MASON K.O., WALTER F.M., BOWYER C.S., STERN R.A., RIEGLER G.R. Astrophys. J., Suppl. Ser., 51, 1-28 (1983) HEAO A-2 soft X-ray source catalog. oTable 1: <H HHMM+DD> N=124
Details on Acronym:   H
   H (HEAO satellite)= (H4) = (HEAO) = (HEAO 4-) Write:<<H HHMM+DDd>> N: 72 Object:(Hard X)  (SIMBAD class: X = X-ray source) Note:All sky. 4 channels in the 13-180keV range. Observations from 1977 August to 1979 January. Data obtained with the UCSD/MIT Hard X-ray and Low-Energy X-ray Instrument on the HEAO 1 satellite. The survey is complete down to an intensity level 1/75 of the Crab Nebulae in the 13-80 keV energy band. 44 sources detected in the 40-80 keV energy band. 7 sources are extragalactic. Ref:=1984ApJS...54..581L byLEVINE A.M. , LANG F.L., LEWIN W.H.G., PRIMINI F.A., DOBSON C.A., DOTY J.P., HOFFMAN J.A., HOWE S.K., SCHEEPMAKER A., WHEATON W.A., MATTESON J.L., BAITY W.A., GRUBER D.E., KNIGHT F.K., NOLAN P.L., PELLING R.M., ROTHSCHILD R.E., PETERSON L.E. Astrophys. J., Suppl. Ser., 54, 581-617 (1984) The HEAO1 A-4 catalog of high-energy X-ray sources. oTable 5: <H HHMM+DDd> N=72
Details on Acronym:   H
   H 08 1994.09.08 (Hubble) ***** Avoid the usage of H, prefer [H29] Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (Hubble) ***** Avoid the usage of H, prefer [H32] Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (Hoffleit) 25-May-1993 - Creation ***** Avoid the usage of H, prefer [H53] Originof the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym:   H
   H (Hodge) ***** Avoid the usage of H, prefer [H60b]
Details on Acronym:   H
   H (Hodge) ***** Avoid the usage of H, prefer [H65] Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (cloud complex labelled H) ***** Avoid the usage of H, prefer [H68] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   H
   H (Hodge) ***** Avoid the usage of H, prefer [H74b] Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (Hodge) ***** Avoid the usage of H, prefer [H76] Originof the Acronym: L (1999ApJ...510..104B)
Details on Acronym:   H
   H (Hodge) ***** Avoid the usage of H, prefer [H77] Originof the Acronym: L (1980A&AS...40...67D)
Details on Acronym:   H
   H (Hawkins) ***** Avoid the usage of H, prefer [H83] Originof the Acronym: L (Veron)
Details on Acronym:   H
   H (Hubble Deep Field) ***** Avoid the usage of H, prefer [HCB98] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   H
   H (Hickson) ***** Avoid the usage of H, prefer HCG Originof the Acronym: L (1993ApJS...85....1N)
Details on Acronym:   H
   H (Holtzman+) ***** Avoid the usage of H, prefer [HFS92] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   H
   H (Hazard+) ***** Avoid the usage of H, prefer [HMT84] Originof the Acronym: L = Found in the literature
Details on Acronym:   H
   H (Hoglund) ***** Avoid the usage of H, prefer NRAO
Details on Acronym:   H
   H (Haddock) ***** Avoid the usage of H, prefer NRL
Details on Acronym:   H
   H (Haro)= H 1- = (Haro 2-). H 2- = (Haro 3-). H 3- = (Haro 6-)
Details on Acronym:   PN H
   PN H Write:<<PN H 1-NN>>
<<PN H 2-NN>>
<<PN H 3-NN>>
<<PN H 4-N>> N: 67+48+2+1 Object:PN + Poss. PN  (SIMBAD class: PN = Planetary Nebula) Stat:is completely incorporated in Simbad Note:List 1: format '1-NN', table 1 in ref. 1952BOTT....1a...1H, H 1-25 and H 1-49 are rejected as PN in 1992, Acker+ catalog.
List 2: format '2-NN', table 2 in ref. 1952BOTT....1a...1H, H 2-9 is a Nova.
List 3: format '3-NN', two objects in ref. 1953BOTT....1h...3H are PN
List4: format '4-N', in ref. 1951PASP...63..14 umbering is continued in 1975ApJS...29..303V, all V* are 'VHK NN' in SIMBAD. o<VHK NN> (Nos 1-45). <[H26] AN> (Nos N1, N2). Auth.:HUBBLE E.P.
Details on Acronym:   [H26]
   [H26] (Hubble, 1926) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   Hanes
   Hanes (Hanes) Write:<<Hanes R-NNN>> Object:Obj.  (SIMBAD class: Unknown = Object of unknown nature) Note:Hanes thesis, 1971: In the format 'R-NNN', the roman number stands for quadrants I to IV.
Some of these objects are found in 1981ApJ...245..416S, Table 4. in source:M 87 = NGC 4486 = Virgo A Auth.:HANES D.A. Originof the Acronym: L (1981ApJ...245..416S)
Details on Acronym:   [HAP2004]
   [HAP2004] (Hatzidimitriou+Antoniou +) ophys. J., 302, 63-66 (1986) IRAS sources associated with shocked gas regions in IC 443. oFig.2: <[HDS86] IC 443A> (Nos IC 443A to IC 443G) Auth.:HUANG Y.-L.+ Ref:=1992ApJ...400..203D byDICKMAN R.L. , SNELL R.L., ZIURYS L.M., HUANG Y.-L. Astrophys. J., 400, 203-213 (1992) Structure and kinematics of dense gas associated with the supernova remnant IC 443. oTable 1: <[HDS86] IC443H> added Ref:=1994ApJ...421..570T byTAUBER J.A. , SNELL R.L., DICKMAN R.L., ZIURYS L.M. Astrophys. J., 421, 570-580 (1994) High-resolution images of shocked molecular clumps in the supernova remnant IC 443. oTables 1, 2: <[HDS86] IC 443AN> (Nos IC443B1 to IC443B4, IC443G1 to IC443G2)
Details on Acronym:   HDW
   HDW (Hartl+Dengel+Weinberger)= (HtDe) Write:<<PN HDW NN>> N: 13 Object:PN  (SIMBAD class: PN = Planetary Nebula) Stat:is completely incorporated in Simbad Note:Th H S
<<PN HDW W3 AN>> N: 3 Object:(X)  (SIMBAD class: X = X-ray source) Stat:is completely incorporated in Simbad in source:W 3 Ref:=2002ApJ...579L..95H byHOFNER P. , DELGADO H., WHITNEY B., CHURCHWELL E., LINZ H. Astrophys. J., 579, 95-98 (2002) X-ray detection of the ionizing stars in ultracompact H II regions. oTable 1: <[HDW2002] W3 DN> (Nos D1-D3). Originof the Acronym: L = Found in the literature
Details on Acronym:   HE
   HE (Hamburg-ESO Survey) Write:<<HE HHMM+DDMMa>> Object:(Opt)  (SIMBAD class: Unknown = Object of unknown nature) Note:1st reference: First ref. from the Hamburg-ESO survey, N=1. Ref:=1991A&A...247L..17W byWISOTZKI L. , WAMSTEKER W., aluminium as tracers of the Galactic Bulge formation. oTable 1 Objects BW-NN not created in Simbad because the authors do not give coordinates. oTables 1, 11, 12: <[LHZ2007] BWc-NN> (Nos 1-13), <[LHZ2007] BW-aN> N=5+6, <[LHZ2007] BN-bN> N=7+5, <[LHZ2007] BN-fN> N=6+7, <[LHZ2007] BL-N> N=7. =E=Catalogue in electronic form as J/A+A/465/799 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [LHZ2010]
   [LHZ2010] (Liu+Ho+Zhang, 2010) Write:<<[LHZ2010] AN>>
<<[LHZ2010] HCN>>
<<[LHZ2010] HCN-B>>
<<[LHZ2010] filament NE>>
<<[LHZ2010] G10-SW>> N: 10+1+1+1+1 Object:Outflow  (SIMBAD class: Outflow) Note:SMA (1.3mm and 0.85mm) and VLA observations of outflows in the massive cluster-forming region G10.6-0.4. in source:GAL 010.6-00.4 Ref:=2010ApJ...725.2190L byLIU H.B. , HO P.T.P., ZHANG Q. Astrophys. J., 725, 2190-2208 (2010) The high-velocity molecular outflows in massive cluster-forming region G10.6-0.4. oFig. 2, Table 3: <[LHZ2010] AN> (Nos R1-R4, B1-B6), <[LHZ2010] HCN> N=1, <[LHZ2010] HCN-B> N=1. Paragr. 3.1: <[LHZ2010] filament NE> N=1, <[LHZ2010] G10-SW> N=1. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   LI
   LI (Leiden IRAS) ***** Avoid the usage of LI, prefer LI-LMC Originof the Acronym: L = Found in the literature
Details on Acronym:   LI
   LI (Leiden IRAS) ***** Avoid the usage of LI, prefer LI-SMC Originof the Acronym: L = Found in the literature
Details on Acronym:   LI-LMC
   LI-LMC (Leiden IRAS-LMC)= (LI) = (LIRL) Write:<<LI-LMC NNNNa>> N: 1891+14 Object:(IR)  (SIMBAD class: IR = Infra-Red source) Note:Results of IRAS pointed observations in four infrared wavelength bands (12, 25, 60 and 100 mu.m)
ref. 1989A&AS...79..105S: Table III: (Nos 1-1823)
Table A2: (Nos 1824-1891) in the periphery of the LMC
1950 coordinates, cross-identif. with IRAS name (IRAS Point Source Catalog). 802 sources are new, not included in either the PSC or SSSC IRAS Catalogs. For maps, use 'Atlas and catalogue' of Schwering+Israel, 1990
ref. 1997A&A...325..585V: The authors introduce a SUFFIX 'b, c, d' in the format, in case of field stars or galaxies, neither of which considered to be the counterpart of the quoted LI-LMC source. See also LI-SMC in source:Magellanic Clouds:LMC = LMC Ref:=1989A&AS...79..105S bySCHWERING P.B.W. Astron. Astrophys., Suppl. Ser., 79, 105-145 (1989) Infrared observations of the Magellanic Clouds. II. The Large Magellanic Cloud. oTable III: <LI-LMC NNNN> (Nos 1-1823). Table A2: <LI-LMC NNNN> (Nos 1824-1891) Ref:=1997A&A...325..585V byVAN LOON J.T. , ZIJLSTRA A.A., WHITELOCK P.A., WATERS L.B.F.M., LOUP C., TRAMS N.R. Astron. Astrophys., 325, 585-600 (1997) Obscured Asymptotic Giant Branch stars in the Magellanic Clouds. III. New IRAS counterparts. oTable 1: <LI-LMC NNNNa> N=14 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   LI-SMC
   LI-SMC (Leiden IRAS-SMC)= (LI) = (LIRS) Write:<<LI-SMC NNN>> N: 249 Object:(IR)  (SIMBAD class: IR = Infra-Red source) Note:Results of IRAS pointed observations in four infrared wavelength bands (12, 25, 60 and 100 mu.m)
Table IV: (Nos 1-219)
Table A2: (Nos 220-249) in SE and SW periphery of the SMC
1950 coordinates, cross-identif. with IRAS name (IRAS Point Source Catalog). 72 sources are new, not included in either the PSC or SSC IRAS Catalogs
For maps, use 'Atlas and catalogue' of Schwering+Israel, 1990
See also LI-LMC in source:Magellanic Clouds:SMC = SMC Ref:=1989A&AS...79...79S bySCHWERING P.B.W. , ISRAEL F.P. Astron. Astrophys., Suppl. Ser., 79, 79-103 (1989) Infrared observations of the Magellanic clouds. I. The Small Magellanic Cloud. oTable IV: <LI-SMC NNN> (Nos 1-219). Table A2: <LI-SMC NNN> (Nos 220-249). Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [LI97]
   [LI97] (Lee+Irwin, 1997) Write:<<[LI97] FNN>> N: 12 Object:Feature  (SIMBAD class: HI = HI (21cm) source) Stat:is completely incorporated in Simbad Note:N=12 arcs and extensions in NGC 3044, (Nos F1-F12). In the format, the letter 'F' stands for Feature. in source:NGC 3044 Ref:=1997ApJ...490..247L byLEE S.-W. , IRWIN J.A. Astrophys. J., 490, 247-262 (1997) Neutral hydrogen in the edge-on spiral galaxy NGC 3044-Global properties and discovery of H I supershells. oTable 4: <[LI97] FNN> (Nos F1-F12) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [LIB2018]
   [LIB2018] (Lewis+Ivison+Best+, 2018) Write:<<[LIB2018] LURGS JHHMMSS.s+DDMMSS>> N: 108 Object:G  (SIMBAD class: Galaxy) Note:APEX LABOCA observations of N=108 dusty star-forming galaxies in the field of 22 galaxies se N> N=6. Auth.:UDALSKI A. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   OGLEIV
   OGLEIV (Optical Gravitational Lensing Exp.) H S (Not yet in Simbad) Write:<<OGLEIV NNA>> N: 21+1 Object:G  (SIMBAD class: Galaxy) Note:Sample of 21 E+A galaxies. The No. 1 as a disturbed companion 1B. Ref:=1996ApJ...466..104Z byZABLUDOFF A.I. , ZARITSKY D., LIN H., TUCKER D., HASHIMOTO Y., SHECTMAN S.A., OEMLER A., KIRSHNER R.P. Astrophys. J., 466, 104-113 (1996) The environment of ``E+A'' galaxies. o(Erratum) erratum vol.516 p.505 (1999) op. 105 : G515 = [HO93] 7- 515 oTable 1: <[ZZL96] NN> (Nos 1-21). e II (B): <Cl* AM 4 IC B-NN> (Nos 1-43). Table II (C): <Cl* AM 4 IC C-NN> (Nos 1-59)
Details on Acronym:   Cl* Antalova 1 DAF
   Cl* Antalova 1 DAF (Dias+Assafin+Florio+) Write:<<Cl* Antalova 1 DAF NNNN>> N: 1122 Object:*inCl Ref:=2006A&A...446..949D byDIAS W.S. , ASSAFIN M., FLORIO V., ALESSI B.S., LIBERO V. Astron. Astrophys., 446, 949-953 (2006) Proper motion dete rmination of open clusters based on the UCAC2 catalogue. oCatalogs pm: <Cl* AAAAAA NNNN DAF NNNN>. =E=Catalogue in electronic form as <J/A+A/446/949/>
Details on Acronym:   Cl* Arp 2 BCF
   Cl* Arp 2 BCF (Buonanno+Corsi+Fusi Pecci+) Write:<<Cl* Arp 2 BCF NNNN>> N: 1586 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1995AJ....109..650B byBUONANNO R. , CORSI C.E., FUSI PECCI F., RICHER H.B., FAHLMAN G.G. Astron. J., 109, 650-662 (199 l. Var. Stars, 5640, 1-None (2005) Newly discovered variable stars in the globular clusters NGC 5634, Arp 2 and Terzan 8. oTable 1: <Cl* NGC 5634 SAW VNN> (Nos V8-V21) added. Table 2: <Cl* Arp 2 SCS VNN> (Nos V1-V12). Table 3: <Cl* Terzan 8 SCS VN> (Nos V1-V4).
Details on Acronym:   Cl* Arp 2 SL
   Cl* Arp 2 SL (Sarajedini+Layden) Write:<<Cl* Arp 2 SL NNN>> N: 896 Object:*inCl Ref:=1997AJ....113..264S bySARAJEDINI A. , LAYDEN A. Astron. J., 113, 264-278 (1997) Reddenings, metallicities, and possible abundance anomalies in young globular clusters. oTable 2: <Cl* Ruprecht 106 SL NNNN> N=3123. Table 3: <Cl* Terzan 7 SL NNN> N=699. Table 4: <Cl* Arp 2 SL NNN> N=896. Table 7: <Cl* Arp 2 SLRR N> N=4 =E=Catalogue in electronic form as <J/AJ/113/264/>
Details on Acronym:   Cl* Arp 2 SLRR
   Cl* Arp 2 SLRR 297 and 353 °. o<Cl Collinder NNN NN>, <Cl Hogg NN NN>, <Cl NGC NNNN NN>, <Cl Pismis NN NN>, <Cl Ruprecht NNN NN>, <Cl Trumpler NN NN>, and <Cl* NGC 5168 MV NN>, <Cl* NGC 5662 MV NN>, <Cl* Pismis 20 MV NN> Auth.:MOFFAT A.F.J.+
Details on Acronym:   Cl* Hogg 14 DAF
   Cl* Hogg 14 DAF (Dias+Assafin+Florio+) Write:<<Cl* Hogg 14 DAF NNN>> N: 144 Object:*inCl Ref:=2006A ys., Suppl. Ser., 10, 135-193 (1973) Southern open star clusters 3 UBV y of stars in galactic cluster fields. oFormat 'NN' for photoelectrically measured stars, Format 'NNN' for photographically measured stars (1st star = No. 101). oCatalogue: <IC NNNN NN> or <Cl* IC NNNN Hoag NN> or <NGC NNNN NN> or <Cl* NGC NNNN Hoag NN> or <Cl Trumpler 2 NN> or (Becker)
Details on Acronym:   IC 2714
   IC 2714 ====>Equivalent to: IC 2714
Details on Acronym:   Cl* IC 2714 BSF
   Cl* IC 2714 BSF (Becker+Svolopoulos+Fang) Write:<<Cl* IC 2714 BSF NNN>> N: 219 Object:*inCl Rem:from the catalogue of Becker+, 1976, Astron. Institut of Basel,
'Kataloge Photographischer und Photoelektrischer Helligkeiten von
25 Galaktischen Sternhaufen im RGU und UcBV system'.
Same lis dry Write:<<Cl* IC 2714 MMU NNN>> N: 14 Object:*inCl Rem:The numbering in this r le 3: <Cl* AAAAA NNNN MMU NNNNN> N=1260 in N=187 clusters. (AAAAA = cluster name). Auth.:MERMILLIOD J.C.+ =E=Catalogue in electronic form as <J/A+A/485/303/>
Details on Acronym:   IC 4996
   IC 4996 Write:<<IC 4996 NN>> N: 79 Object:*inCl Ref:=1967VeBon..76....0V byVAN SCHEWICK H. Veroeff. Astron. Inst. Bonn, -1-None (1967) Untersuchungen uber die Eigenbewegungen von Sternhaufen XIII. IC 4996, NG 548 (1996) BVRI CCD photometry of the open cluster IC 4996. oTable 1: <Cl*
Details on Acronym:   Cl* Melotte 20 SHBJ
   Cl* Melotte 20 SHBJ (Stauffer+Hartmann+Burnham+Jones) A MARTIN E.L. Nature, 377, 129-131 (1995) Discovery of a brown dwarf in the Pleiades star clust er. o<Cl* Melotte 22 Teide 1> N=1 Ref:=1998ApJ...499L..61M MU Rem:The numbering in this reference is the same as Auth.:WALKER A.R.
Details on Acronym:   Cl* NGC 1835 LE
   Cl* NGC 1835 LE (Lloyd Evans) Write:<<Cl* NGC 1835 LE N>> N: 4 Object:*inCl Ref:=1980MNRAS.193...87L byLLOYD EVANS T. Mon. Not. R. Astron. Soc., 193, 87-96 (1980) Red stars in Magellanic Cloud globular clusters. oTable 1: <Cl* NGC NNNN LE NN>, <C GC 188 PKM NNNN> (Nos 1-9596). =E=Catalogue in electronic form as <J/AJ/126/2922/>
Details on Acronym:   Cl* NGC 188 R
   Cl* NGC 188 R (Rufener) Write:<<Cl* NGC 188 R NNN>> N: 5 among 105 Object:*inCl Ref:=1971A&AS....3..181R byRUFENER F.G. Astron. Astrophys., Suppl. Ser., 3, 181-252 (1971) Catalogue of stars measured in the Geneva Observatory photometric system. oCata col(1O), p. 226: the objects are named 'Cl Upgren 1 NN' by Mermilliod J.-C. in the HIC catalog. o, IRIARTE B., MITCHELL R.I., HALLAM K.L., SHARPLESS S. Publ. U.S. Naval Obs. Second Serie, 17, 343-542 (1961) Photometry of stars in galactic cluster fields. oFormat 'NN' for photoelectrically measured stars, Format 'NNN' for photographically measured stars (1st star = No. 101). oCatalogue: <IC NNNN NN> or <Cl* IC NNNN Hoag NN> or <NGC NNNN NN> or J Mon. Not. R. Astron. Soc., 193, 87-96 (1980) Red stars in Magellanic Cloud globular c 122 (1990) The asymptotic giant branch of Magellanic Cloud clusters. oin ref list BLANCO 198 fat + Vogt ====>Equivalent to: NGC 2421
Details on Acronym:   Cl* NGC 2421 PR
   Cl* NGC 2421 PR 7 (C0749-317). oTable 2: <Cl* NGC 2671 P NN> (Nos 1-62). Table 3: <Cl* Haffner 17 P NNN> (Nos 1-123, No. 62 missing). Auth.:PEDREROS M.H.
Details on Acronym:   NGC 2682
   NGC 2682 Write:<<NGC 2682 NNN>> N: 295 Object:*inCl Rem:Fagerholm, 1906, PhD Thesis Upssala Univ.
Details on Acronym:   Cl* NGC 2682 Barn
   Cl* NGC 2682 Barn () Barnard Write:<<Cl* NGC 2682 Barn NN>> N: 41 Object:*inCl Ref:=1931PYerO...6....1B byBARNARD E.E. Publ. Ye GC 3114 PPM (Paunzen+Pintado+Maitzen)
Details on Acronym:   Cl* NGC 3532 Fern
   Cl* NGC 3532 Fern (Fernandez+) Write:<<Cl* NGC 3532 Fern NNN>>
<<Cl* NGC 3532 Fern A>> N: 700+1 Object:*in NGC 5466 SAW VNN> (Nos V37-V38) added, <Cl* NGC 5466 FLG N> (Nos 1-3). 09 Auth.:ORSATTI A.M.+ =E=Catalogue in electronic form as <J/A+A/471/165/>
Details on Acronym:   Cl* NGC 5606 Vz
   Cl* NGC 5606 Vz (Vazq) N: 2 Object:*inCl Ref:=2001AJ....121..318A byALVES D.R. , BOND H.E., ONKEN GC 6124
Details on Acronym:   Cl* NGC 6124 Ko
   Cl* NGC 6124 Ko (Koelbloed) ====>Equivalent to: NGC 6124
Details on Acronym:   Cl* NGC 6124 MMU
   Cl* NGC 6124 MMU (Mermillod+Mayor+Udry) Write:<<Cl* NGC 6124 MMU NNN>> N: 8 Object:*inCl Rem:The numbering in this reference is the same as the one used in the WEBDA
database at the date of the publication of the paper. Ref:=2008A&A...485..303M byMERMILLIOD J.C. , MAYOR M., UDRY S. Astron. Astrophys., 485, 303-314 (2008) Red giants in open clusters. XIV. Mean radial velocities for 1309 stars and 166 open clusters tars and 166 open clusters. oStar 599 in NGC 2355 = Cl* NGC 2355 ALC 599 (from the unpublis Ferraro + Clementini + Fusi Pecci+ Write:<<Cl* NGC 6171 FCF NNNN>> N: 1677 Object:*inCl (Sawyer-Hogg) Proper motion determination of open clusters based on the UCAC2 catalogue. oCatalogs pm: <Cl* AAAAAA NNNN DAF NNNN>. =E=Catalogue in electronic form as <J/A+A/446/949/>
Details on Acronym:   Cl* NGC 6281 FF
   Cl* NGC 6281 FF (Feinstein+Forte) ====>Equivalent to: NGC 6281
Details on Acronym:   Cl* NGC 6281 MMU
   Cl* NGC 6281 MMU (Mermillod+Mayor+Udry) Write:<<Cl* NGC 6281 MMU N>> N: 2 Object:*inCl Rem:The numbering in this reference is the same as the one used in the WEBDA
database at the date of the publication of the paper. Ref:=2008A&A...485..303M GC 6341 SH NNN> (Nos 1-108, 203-509). Table IV (e): <Cl* NGC 7089 SH NN> N=35 among (Nos 5-81). Table IV (f): <Cl* NGC 5272 SH NN> N=59 among (Nos 1-74). Table IV (g): <Cl* NGC 5904 SH NN> (Nos 1-56). Table IV (h): <Cl* NGC 7078 NN> (Nos 1-74). Auth.:STETSON P.B.+
Details on Acronym:   Cl* NGC 6341 SK
   Cl* NGC 6341 SK (Sandage+Katem) Write:<<Cl* NGC 6341 SK NNNNNA>> N: 375 Object:*inCl Rem:Tables 1, 3:
Format 'NNNNNA' (6 digits):
The first digit is a Roman digit for ring (III or IV),
Translated by '3' or '4'.

the second digit is a subdivision of the ring (ex. ring IV-2),
the letter at the en A byARMANDROFF T.E. Astron. J., 96, 588-634 (1988) Color-magnitude diagrams for six metal-rich, low-latitude globular clusters. oTable II: <Cl* NGC 104 A NN> N=47, Table III: <Cl* NGC 6316 A NNN> N=808, Table IV: <Cl* NGC 6342 A NNN> N=306, Table V: <Cl* NGC 6486 A NNN> N=285, Table VI: <Cl* NGC 6539 A NNN> N=445, Table VII: <Cl* Palomar 8 A NNN> N=425, Table VIII: <Cl* NGC 6760 A NNN> N=550
Details on Acronym:   Cl* NGC 6342 OVR
   Cl* NGC 6342 OVR (Origlia+Valnti+Rich) Write:<<Cl* NGC 6342 OVR N>> N: 4 Object:*inCl Ref:=2005MNRAS.356.1276O (Piatti+Sarajedini+Geisler+) Write:<<Cl* NGC 643 PSG NNNN>> N: 1812 Object:*inCl Ref:=2007MNRAS.382.1203P byPIATTI A.E. , SARAJEDINI A., GEISLER D., GALLART C., WISCHNJEWSKY M. Mon. Not. R. Astron. Soc., 382, 1203-1212 (2007) Five young star clusters in the outer region of the Small Magellanic Cloud. oTable 2: <Cl* Lindsay 106 PSG NNNN> (Nos 1-1154). Table 3: <Cl* Lindsay 108 PSG NNNN> (Nos -3234). Table 4: <Cl* NGC 643 PSG NNNN> (Nos 1-1812). Table 5: <Cl* Lindsay 114 PSG NNNN> (Nos 1-2193). Table 6: <Cl* NGC 796 PSG NNNN> (Nos 1-1360). ., 122, 2600-2626 (2001) Variable stars in the unusual, metal-rich, globular cluster NGC 6441. o(Erratum) erratum vol. 125, p. 2751 (2003) oTable 2: <Cl* NGC 6441 SAW VNNN> (Nos V51-V104) added. Ref:=2003AJ....126.1381P byPRITZL B.J. , SMITH H.A., STETSON P.B., CATELAN M., SWEIGART A.V., LAYDEN A.C., RICH R.M. Astron. J., 126, 1381-1401 (2003) Hubble space telescope snapshot study of variable stars in globular clusters: the inner region of NGC 6441. oTable 8 : Star V4 in NGC 7492 is Cl* NGC 7492 C G. oTable 5: <Cl* NGC 6441 SAW VNNN> s or http://menhir.pd.astro.it o<Cl* NGC NNNN PKD NNNNN>, <Cl* IC NNNN PKD NNNNN>, for N=74 Cl* at CDS + 23 in Piotto database only. =E=Catalogue in electronic form as <J/A+A/391/945/>
Details on Acronym:   Cl* NGC 6469 DAF
   Cl* NGC 6469 DAF (Dias+Assafin+Florio+) Write:<<Cl* NGC 6469 DAF NN>> N: 80 Object:*inCl Ref:=2006A&A...446..949D byDIAS W.S. , ASSAFIN M., FLORIO V., ALESSI B.S., LIBERO V. Astron. Astrophys., 446, 949-953 (2006) Proper motion determination of open clusters based on the UCAC2 catalogue. oCatalogs pm: <Cl* AAAAAA NNNN DAF NNNN>. rmat A. Table III: format NNN Ref:=1983A&AS...52..105A byALCAINO G. Astron. Astrophys., Suppl. Ser., 52, 105-113 (1983) The globular cluster NGC 6544. oTable I: <Cl* NGC 6544 ALC A> (Nos A-U, O missing). Table III: <Cl* NGC 6544 ALC NNN> (Nos 1-164).
Details on Acronym:   Cl* NGC 6544 Haz
   Cl* NGC 6544 Haz (Hazen) Write:<<Cl* NGC 6544 Haz a>>
<<Cl* NGC 6544 Haz VN>>
<<Cl* NGC 6544 Haz FN>>
<<Cl* NGC 6544 Haz LPM>> N: 9+2+2+1 Object:*inCl Rem:star LPM (Large Proper Motion). Ref:=1993AJ....106.1055H byHAZEN M.L. Astron. J., 106, 1055-1058 (1993) The variable stars in the field of the globular cluster NGC 6544. oTable 1: <Cl* NGC 65 44 HAZ a> (Nos b-f, i-l). Table 3: <Cl* NGC 6544 HAZ VN> (Nos V1-V2). Table 4: <Cl* NGC 6544 HAZ FN> (Nos F1-F2). Table 5: <Cl* NGC 6544 HAZ LPM> N=1.
Details on Acronym:   Cl* NGC 6544 PKD
   Cl* NGC 6544 PKD (Piotto+King+Djorgovski+) Write:<<Cl* NGC 6544 PKD NNNNN>> N: about 4400 Object:*inCl Ref:=2002A&A...391..945P byPIOTTO G. , KING I.R., DJORGOVSKI S.G., SOSIN C., ZOCCALI M., SAVIANE I., DE ANGELI F., RIELLO M., RECIO-BLANCO A., RICH R.M., MEYLAN G., RENZINI A. Astron. Astrophys., 391, 945-965 (2002) HST color-ma N=187 clusters. (AAAAA = cluster name). =E=Catalogue in electronic form as <J/A+A/485/303/>
Details on Acronym:   Cl* NGC 6553 GOM
   Cl* NGC 6553 GOM (Guarnieri+Ortolani+Montegriffo+) Write:<<Cl* NGC 6553 GOM NNNNN>> N: 1426 Object:*inCl Rem:Nos 1 to 2197 belong to the WFPC2 PC chip,
20001 to 26240 to the WFPC2 chip 2
30001 to 39545 to the WFPC2 chip 3
40001 to 48688 to the WFPC2 chip 4 Ref:=1998A&A...331...70G byGUARNIERI M.D. , ORTOLANI S., MONTEGRIFFO P., RENZINI A., BARBUY B., BICA E., MONETI A. Astron. Astrophys., 331, 70-80 (1998) Infrared array photometry of bulge globular clusters. I. Combined ground b ased JK and HST VI photometry of NGC 6553. oAppendix: <Cl* NGC 6553 GOM NNNNN> N=1426 among (Nos 1-2197, 20001-26240, 30001-39545, 40001-48688) =E=Catalogue in electronic form as <J/A+A/331/70/>
Details on Acronym:   Cl* NGC 6553 Har
   Cl* NGC 6553 Har (Hartwick) Write:<<Cl* NGC 6553 Har NN>>
<<Cl* NGC 6553 Har R-NNN>> N: 48+166 Object:*inCl Rem:Format R-NNN where 'R' stands for quadrant I to IV.

This format can also be written 'NNNN' with 4 digits. Ref:=1975PASP...87...77H byHARTWICK F.D.A. Publ. Astron. Soc. Pac., Ref:=2007A&A...462..245G byGUARCELLO M.G. , PRISINZANO L. NDERS W.L.
Details on Acronym:   Cl* NGC 6633 VKP
   Cl* NGC 6633 VKP (Vasilevskis+Klemola+Preston) Write:<<Cl* NGC 6633 VKP NNN>> N: 207 Object:*inCl Ref:=1958AJ.....63..387V byVASILEVSKIS S. , KLEMOLA A., PRESTON G. Astron. J., 63, 387-395 (1958) Relative proper motions of stars in the region of the open cluster NGC 6633. oTable II: <Cl* NGC 6633 VKP NNN> (Nos 1-207).
Details on Acronym:   Cl* NGC 6637 FFG
   Cl* NGC 6637 FFG (Ferraro+Fusi Pecci+Guarnieri+) Write:<<Cl* NGC 6637 FFG NNNN>> N: 1516 Object:*inCl Rem:Table 1(b): Optical data. Ref:=1994MNRAS.266..829F byFERRARO F.R. , NTI E.+ =E=Catalogue in electronic form as <J/AJ/133/1287/>
Details on Acronym:   Cl* NGC 6638 VOF
   Cl* NGC 6638 VOF (Valenti+Origlia+Ferraro) Write:<<Cl* NGC 6638 VOF NNNNN>> N: 10255 Object:*inCl Ref:=2005MNRAS.361..272V byVALENTI E. , ORIGLIA L., FERRARO F.R. Mon. Not. R. Astron. Soc., 361, 272-282 (2005) Near-infrared photometry of four metal-rich bulge globular clusters: NGC 6304, 6569, 6637 and 6638. oCatalog: <Cl* NGC 6304 VOF NNNN> (Nos 1-9103), <Cl* NGC 6569 VOF NNNNN> (Nos 1-10182), <Cl* NGC 6637 VOF NNNNN> (Nos 1-12295), <Cl* NGC 6638 VOF NNNNN> (Nos 1-10255).
Details on Acronym:   Cl* NGC 6642 H
   Cl* NGC 6642 H Auth.:HAZEN-LILLER M.L.
Details on Acronym:   Cl* NGC 6652 OBB
   Cl* NGC 6652 OBB (Ortolani+Bica+Barbuy) Write:<<Cl* NGC 6652 OBB NNNN>> N: 2226 Object:*inCl Ref:=1994A&A...286..444O byORTOLANI S. , BICA E., BARBUY B. Astron. Astrophys., 286, 444-448 (1994) The globular cluster NGC 6652. oTables 2, 3: <Cl* NGC 6652 OBB NNNN> (Nos 1-2226). =E=Catalogue in electronic form as <J/A+A/286/444/>
Details on Acronym:   Cl* NGC 6652 PKD
   Cl* NGC 6652 PKD (Piotto+King+Djorgovski+) Write:<<Cl* NGC 6652 PKD NNNNN>> Object:*inCl Ref:=2002A&A...391..945P byPIOTTO G. , KING I.R. added. Table A15: <NGC 2808 NNN> (Nos 1-347), <Cl* NGC NNNN Har NNNA> N=99+49+267+394+327 (for NGC 6325, 6517, 6681, 6715, 6809), <Cl* NGC NNNN Har R-NNNA> N=342+301+344+334+733 (for NGC 4590, 5694, 5824, 6864, 7089). Auth.:HARRIS W.E.
Details on Acronym:   Cl* NGC 6715 I
   Cl* NGC 6715 I (Ibata) Write:<<Cl* NGC 6715 I NN>> Object:*inCl Ref:=1999AJ....118.1245B byBROWN J.A. , WALLERSTEIN G., GONZALEZ G. Astron. J., 118, 1245-1251 (1999) Elemental abundances in five stars in M54, a globular cluster associated with the Sagittarius galaxy. oT.1: from R. Ibata, unpublished. oTable 1: <Cl* NGC Cl* NGC NNNN MVF NNNNN> in fields around 8 clusters.
Details on Acronym:   Cl* NGC 6830 MVF
   Cl* NGC 6830 MVF (Moffat+Vogt, Feldgebiet) Write:<<Cl* NGC 6830 MVF NNNNN # 5 digits>> N: 636 O *inCl Rem:N=636 among (Nos 11001-44038) * in the field around NGC 6830,
always a 5 digits format Ref:=1974VeBoc...2....1M byMOFFAT A.F.J. , VOGT N. Veroeff. Astron. Inst. Ruhr-Univ. Bochum, 2, 1-None (1974) Photographische UBV-H elligkeiten in 14 jungen Sternhaufen der nordlichen Milchstrasse. oformat 'MV' for stars in 'Haufengebiet', format inCl Ref:=1973PDDO....3....6S bySAWYER HOGG H. Publ. David Dunlap Obs., 3, ion of the open cluster NGC 7039. o<Cl* NGC 7039 ZS NNN> (Nos 35-40) and N=13 among (80-333).
Details on Acronym:   Cl* NGC 7044 A
   Cl* NGC 7044 A (Aparicio+) ====>Equivalent to: Cl* NGC 7044 AAD
Details on Acronym:   Cl* NGC 7044 AAD
   Cl* NGC 7044 AAD (Aparicio+Alfaro+Delgado+) Write:<<Cl* NGC 7044 AAD NNNN>> N: 896 among 1004 Object:*inCl Ref:=1993AJ....106.1547A byAPARICIO A. , ALFARO E.J., DELGADO A.J., RODRIGUEZ-ULLOA J.A., CABRERA-CANO J. Astron. J., 106, 1547-1560 (1993) The i he a Fente Multiple Write:<<Cl* NGC 7078 SFM NN>> N: 55 Object:*inCl Ref:=1994ExA DOI 10.1086/168415 bySANDAGE A. Astrophys. J., 350, 603-630 (1990) Th e vertical height of the horizontal branch: the range in the absolute magnitudes of RR Lyrae stars in a given globular cluster. oTable 2: From an unpublished catalog of Sandage+, 1968 NGC 7243 M (Maevers) Write:<<Cl* NGC 7243 M NNN>> N: 133 Object:*inCl Ref:=1940 tions. Ref:=1961MNRAS.122..363C byCUFFEY J. S N> (Nos 1-3), <Cl* Palomar 3 HS N> (Nos 1, 3), <Cl* Palomar 11 HS N> (Nos 1-3), <Cl* Palomar 12 HS N> (Nos 3, 5), <Cl* Palomar 13 HS N> (Nos 1-2). Table 6: <Cl* Palomar 14 HS NN> (Nos 1-62). Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* Palomar 12 KHG
   Cl* Palomar 12 KHG (Kayser+Hilker+Grebel) Write:<<Cl* Palomar 12 KHG NN>> N: 25 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2008A&A...486..437K byKAYSER A. , HILKER M., GREBEL E. + Ref:=2001AJ....121..935S bySIEGEL M.H. , MAJEWSKI S.R., CUDWORTH K.M., TAKAMIYA M. Astron. J., 121, 935-950 (2001) A cluster's last stand: the death of Palomar 13. oTables 3, 4: <Cl* Palomar 13 SMC NNNN> N=421 among (Nos 1-3680). Table 5: <Cl* Palomar 13 BSSC N> (Nos 8-9) added. =E=Catalogue in electronic form as <J/AJ/121/935/>
Details on Acronym:   Cl* Palomar 13 CDM
   Cl* Palomar 13 CDM (Cote+Djorgovski+Meylan+) Write:<<Cl* Palomar 13 CDM NNN>> N: 4+70 Object:*inCl Ref:=200

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