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

Result of query: info cati SA FFF$



.
 
 on Nebula Cluster.
oTable 1: <[H97b] NNNNN> N=829 among (Nos 10003-11115) added.
 Auth.:HERBST W.+
   Ref:=2009A&A...502..883R
     byRODRIGUEZ-LEDESMA M.V.
, MUNDT R., EISLOEFFEL J.
 Astron. Astrophys., 502, 883-904 (2009)

    Rotational studies in the Orion nebula cluster: from solar mass stars
    to brown dwarfs.
oTable 1: <[H97b] NNNNN> N=1668 among (Nos 20000-21668).
=E=Catalogue in electronic form as J/AJ/113/1733
=E=Catalogue in electronic form as J/A+A/502/883

Details on Acronym:   [H98]
   [H98] (Hojaev, 1998)= ([H98a]) Write:<<[H98] BH-a NN>>
<<[H98] SBH-a NN>> N: 20+18 Object:Em*  (SIMBAD class: Em* = Emission-line Star) Stat:is completely incorporated in Simbad Note:Table 2: N=20 Byurakan H-alpha emission stars, format 'BH-a NN'. Table 3: N=18 Byurakan Suspected H-alpha emission stars, format 'SBH-a NN' Ref:=1998PASA...15..152H byHOJAEV A.S. Publications - Astron. Soc. Australia, 15, 152-154 (1 III. The dynamically young merger remnant NGC 3921. oTable 3: <S96 NN> (Nos 1-30), Table 5: <S96 GN> (Nos G1-G8) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S96b]
   [S96b] (Stein, 1996)= (St) Write:<<[S96b] ACO NNNN NNN>>
<<[S96b] ACO SNNN NN>>
<<[S96b] Cl 1322-30 NN>>
<<[S96b] Fld NN NN>> N: 751+111 Object:G in ClG  (SIMBAD class: GinCl = Galaxy in Cluster of Galaxies) Note:Tables 1, 2 only available in electronic form
Table 1: redshifts and type inside 15 clusters: ACO S 301: format 'ACO S301 NN', (Nos 1-22)
ACO 400: format 'ACO 400 NN', (Nos 1-35)
ACO 1016: format 'ACO 1016 NN', (Nos 1-37)
ACO 1060: format 'ACO 1060 NN', (Nos 1-72)
ACO S 639: format 'ACO S639 NN' (Nos 1-36)
ACO 3526: format 'ACO 3526 NN', (Nos 1-49)
ACO S 721: format 'ACO S721 NN' (Nos 1-40)
ACO 3556: format 'ACO 3556 NN', (Nos 1-56)
ACO 1736: format 'ACO 1736 NN', (Nos 1-76)
ClG 1322-30: format 'Cl 1322-30 NN', (Nos 1-27)
ACO 3558: format 'ACO 3558 NNN', (Nos 1-144)
ACO S 805: format 'ACO S805 NN' (No s 1-31)
ACO 3733: format 'ACO 3733 NN', (Nos 1-39)
ACO 3880: format 'ACO 3880 NN', (Nos 1-30)
ACO 4038: format 'ACO 4038 NN', (Nos 1-57)
Table 2: redshifts and type outside the clusters: Field 44: format 'Fld 44 NN', (Nos 1-52)
Field 77: format 'Fld 77 NN', (Nos 1-30)
Field 79: format 'Fld 79 NN', (Nos 1-29) in source:ACO S 301 in source:ACO 400 in source:ACO 1016 in source:ACO 1060 in source:ACO S 639 in source:ACO 3526 = Centaurus Cluster in source:ACO S 721 in source:ACO 3556 in source:ACO 1736 in source:ClG 1322-3027 in source:ACO 3558 in source:ACO S 805 in source:ACO 3533 in source:ACO 3880 in source:ACO 4038 Ref:=1996A&AS..116..203S bySTEIN P. Astron. Astrophys., Suppl. Ser., 116, 203-209 (1996) Structure and kinematics of galaxy clusters. I. The redshift catalogue. oTable 1: <[S96b] ACO NNNN NNN>, <[S96b] ACO SNNN NN>, <[S96b] Cl 1322-30 NN> N=751. Table 2: <[S96b] Fld NN NN> N=111 =E=Catalogue in electronic form as J/A+AS/116/203 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S96c]
   [S96c] (Sakamoto, 1996) Write:<<[S96c] CN>> N: 8 Object:Clump  (SIMBAD class: PartofG = Part of a Galaxy) Stat:is completely incorporated in Simbad in source:NGC 4414 Ref:=1996ApJ...471..173S bySAKAMOTO K. Astrophys. J., 471, 173-189 (1996) Molecular gas disk in the flocculent spiral galaxy NGC 4414. oTable 4: <[S96c] CN> (Nos C1-C8) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S96d]
   [S96d] (Schweitzer, 1996) Write:<<[S96d] NNNN>> N: 32 Object:*  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:N=32 stars (CMD outliers) from Schweitzer Ph.D. Thesis, 1996, Wisconsin. Ref:= 2001AJ....122.3106E byESKRIDGE P.B. , SCHWEITZER A.E. Astron. J., 122, 3106-3114 (2001) Analysis of a proper-motion-selected sample of stars in the Ursa Minor dwarf spheroidal galaxy. oTable 1: Stars from Schweitzer A.E., Ph.D. Thesis, 1996, Wisconsin. Table 2: density excesses are not considered as objects in SIMBAD. oTable 1: <[S96d] NNNN> N=32 among (Nos 152-1859). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S97]
   [S97] (Saurer, 1997) Write:<<[S97] NNN>> N: 110 Object:*  (SIMBAD class: Star) Note:N=110 stars around PN K 3-82
Fig.7: Finding Chart Ref:=1997A&A...328..641S bySAURER W. Astron. Astrophys., 328, 641-648 (1997) A study of the planetary nebula K3-82. oobjects from Table 3 not in SIMBAD (no position) oTable 3: <[S97] NNN > (Nos 1-110) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S98]
   [S98] (Saurer, 1998)= [S98a] Write:<<[S98] NNN>> N: 130 Object:*  (SIMBAD class: Star) Note:N=130 stars around PN M 1-79
Fig.C1: Finding Chart Ref:=1998MNRAS.299...51S bySAURER W. Mon. Not. R. Astron. Soc., 299, 51-59 (1998) Distance determination and low-resolution spectroscopy of the planetary nebula M1-79. oTable B1: <[S98] NNN> (Nos 1-130). =E=Catalogue in electronic form as J/MNRAS/299/1 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S98a]
   [S98a] (Saurer, 1998) ***** Avoid the usage of [S98a], prefer [S98] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S98b]
   [S98b] (Songalai, 1998) Write:<<[S98b] HHMM+DDd>>
<<[S98b] HHMM+DDMM>> N: 13 Object:QSO  (SIMBAD class: QSO = Quasar) Stat:is completely incorporated in Simbad Ref:=1998AJ....115.2184S bySONGAILA A. Astron. J., 115, 2184-2205 (1998) The redshift evolution of the metagalactic ionizing flux inferred from metal line ratios in the Lyman forest. oTable 1: <[S98b] HHMM+DDd>, <[S98b] HHMM+DDMM>, N=13. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S99]
   [S99] (Sandell, 1999)= (MM) = [S99a] Write:<<[S99] MM Na>> N: 5 Object:(mm)  (SIMBAD class: Radio(mm) = millimetric Radio-source) Stat:is completely incorporated in Simbad Ref:=1999A&A...343..281S bySANDELL G. Astron. Astrophys., 343, 281-286 (1999) (Sub)mm continuum observations of NGC 6334A. o[S99] MM 2 is associated wi th [HG83] IRS-IV-3. oTable 1: <[S99] MM Na> (Nos 1a-1b, 2-4). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S99a]
   [S99a] (Sandell, 1999) ***** Avoid the usage of [S99a], prefer [S99] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S99b]
   [S99b] (Stanton, 1999) (Not yet in Simbad) Write:<<[S99b] NNN>>
<<[S99b] a>> N: 19+23 Object:*  (SIMBAD class: Star) Note:M ap Fig.1: N=19 comparison stars among (Nos 75-153), and N=23 unknown stars among (Nos a-z), in the field of SS Cyg. Ref:=1999JAVSO..27...97S bySTANTON R.H. J. Am. Assoc. Variable star obs., 27, 97-112 (1999) Visual magnitudes and the "average observer": the SS Cygni field experiment. oTable 2: <[S99b] NNN> N=19 among (Nos 75-153), <[S99b] a> N=23 among (Nos a-z). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S99c]
   [S99c] (Singh, 1999) Write:<<[S99c] NN>> N: 16 Object:(X)  (SIMBAD class: X = X-ray source) Stat:is completely incorporated in Simbad Note:ROSAT HRI observations of NGC 1365 and NGC 4051.
N=16 new X-ray sources are detected. (Nos 1-13) in NGC 1365 field, (Nos 14-16) in NGC 4051 field. in source:NGC 1365 in source:NGC 4051 Ref:=1999MNRAS.309..991S bySINGH K.P. Mon. Not. R. Astron. Soc., 309, 991-1006 (1999) High-resolution X-ray imaging observations of two low-luminosity Seyfert galaxies. oTable 3: <[S99c] NN> (Nos 1-16). 12.16 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [S99d]
   [S99d] (Skiff, 1999) Write:<<[S99d] NGC 2841 N>> N: 5 Object:*  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:Comparison stars in the field of NGC 2841. Stars numbering given by Skiff, 1999, (Nos 1-5): 1999, VSNET Alerts 2917, 2919, 2937, and ftp://ftp.lowell.edu/pub/bas/starcats/loneos.phot. Only (Nos 2-4) in Ref. 2000A&A...361...63T. Ref:=2000A&A...361...63T byTOTH I. , SZABO R. Astron. Astrophys., 361, 63-67 (2000) The Type Ia SN 1999by in NGC 2841: near-maximum BV(RI)_c photometry and the multicolor light-curve shape (MLCS) method. oFig.1: <[S99d] NGC 2841 N> (Nos 2-4). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   SA
   SA (Selected Area) Originof the Acronym: L = Found in the literature Eichfelder 1-19. o<BSD FF-NNNN> Auth.:SCHWASSMANN A.+ Ref:=1938BSD...C02....0S bySCHWASSMANN A. , VAN RHIJN P.J. Hamburger Sternwarte Bergedorf, 2, 0-None (1938) Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 20-43. o<BSD FF-NNNN> Ref:=1947BSD...C03....0S bySCHWASSMANN A. , VAN RHIJN P.J. Hamburger Sternwarte Bergedorf, 3, 0-None (1947) Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteyn Eichfelder 44-67. o<BSD FF-NNNN> 1.01.86 10.01.21 Ref:=1951BSD...C04....0S bySCHWASSMANN A. , VAN RHIJN P.J. Hamburger Sternwarte Bergedorf, 4, 0-None (1951) Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 68-91. o<BSD FF-NNNN> Ref:=1953BSD...C05....0S bySCHWASSMANN A. , VAN RHIJN P.J. Hamburger Sternwarte Bergedorf, 5, 0-None (1953) Bergedorf Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 92-115. o<BSD FFF-NNNN>
Details on Acronym:   SA
   SA (Selected Area) D ***** Avoid the usage of SA, prefer BSD
Details on Acronym:   SA
   SA (Structure in ACO) G99] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [SAM91]
   [SAM91] (Salzer+Di Serego Alighieri+Matteucci+, 2012) Write:<<[SAM91] SN>> N: 4 Object:*  (SIMBAD class: Star) Note:ESO KPNO observations of N=4 stars in the field of the optical dwarf galaxy NAME DW 1225+0152. in source:NAME DW 1225+0152 Ref:=1991AJ....101.1258S bySALZER J.J. , DI SEREGO ALIGHIERI S., MATTEUCCI F., GIOVANELLI R., HAYNES M.P. Astron. J., 101, 1258-1274 (1991) The optical counterpart to the large H I cloud in Virgo. oFig. 4, Table 1: <[SAM91] SN> (Nos S1-S4). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [SAM95]
   [SAM95] (Seiradakis+Avgoloupis+Mavridis+, 1995) Write:<<[SAM95] UV CET N>>
<<[SAM95] YY GEM N>>
<<[SAM95] AD LEO N>>
<<[SAM95] BY DRA N>>
<<[SAM95] EV LAC N>>
<<[SAM95] EQ PEG N>> N: 5+2+1+1+4+3 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Stat:is completely incorporated in Simbad Note:Radio-sources in the vicinity of flare stars. Ref:=1995AA...29 9375 N: 16588+28008 Object:G  (SIMBAD class: Galaxy) Note:The Shapley Optical Survey (SOS) is a photometric study covering a ∼2-deg2 region of the Shapley supercluster core at z∼0.05 in two bands (B and R).
Use of archival ESO/MPI 2.2m telescope imaging data. Ref:=2006MNRAS.368..109M byMERCURIO A. , MERLUZZI P., HAINES C.P., GARGIULO A., KRUSANOVA N., BUSARELLO G., LA BARBERA F., CAPACCIOLI M., COVONE G. Mon. Not. R. Astron. Soc., 368, 109-120 (2006) Shapley Optical Survey - I. L M 82 ? oTable 2: radio counterpart = [MPW94] oTable 2: <[SSW99] XN> (Nos X1-X4). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   SSWMW
   SSWMW (Strom+Strom+Wolff+Morgan+Wenz)= ([SSW86]) Write:<<SSWMW HH NNN NNN>>
<<SSWMW HH NN-NN NN>>
<<SSWMW HH NN,NN NN>>
<<SSWMW HH 34North NN>>
<<SSWMW HH 14-4,14-6 NN>>
<<SSWMW Hubble 4 N>>
<<SSWMW Haro 6-NN NN>>
<<SSWMW L 1551 NN>>
<<SSWMW HL,XZ Tau NN>>
<<SSWMW AA CCC NN>>
<<SSWMW GGD 34-35 NN>>
<<SSWMW GGD 18 NN>>
<<SSWMW LkHa 233 NN>>
<<SSWMW MWC 1080 NN>> HH 43,38 8 N: 1018 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Note:Tables 3 to 28: imaging survey of 38 regions.
Maps figs 7 to 42 Ref:=1986ApJS...62...39S bySTROM K.M. , STROM S.E., WOLFF S.C., MORGAN J., WENZ M. Astrophys. J., Suppl. Ser., 62, 39-80 (1986) Optical manifestations of mass outflows from young stars

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