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

Result of query: info cati W$
  A High-Sensivity Survey of the North Polar Galactic Region at 1415    MHz.
o<Ohio A DNN.N>, <Ohio A -DNN.N> lettre 'A' from 'B' to 'Z' omitting    'O'
 Auth.:SCHEER D.J.+
   Ref:=1975AJ.....80..759R
     byRINSLAND C.P.
, DIXON R.S., KRAUS J.D.
 Astron. J., 80, 759-770 (1975)

    Ohio Survey supplement 2.

o<Ohio A DNN.N>, <Ohio A -DNN.N> lettre 'A' from 'B' to 'Z' omitting    'O'

Details on Acronym:   OV
   OV (Oklahoma univ., Variable *) Write:<<SV* OV NN>> Object:V*  (SIMBAD class: V* = Variable Star) Rem:V* Nomenclature.
Details on Acronym:   OVH
   OVH (Ohio univ., V stands for 20st hour of RA, H stands for High-Vel.) ***** Avoid the usage of OVH, prefer Ohio Originof the Acronym: L = Found in the literature
Details on Acronym:   SMC
   SMC (Streaming Motions of Abell Clusters) Originof the Acronym: A = Assigned by the author(s) oTable 1: <MCC NNN> (Nos 877-895) Auth.:VYSSOTSKY A.N. =E=Catalogue in electronic form as III/13
Details on Acronym:   [VYT85]
   [VYT85] (van den Bergh+Younger+Turner, 1985) Write:<<[VYT85] AA CCC A>> N: 56 Object:*  (SIMBAD class: Star) Note:Cerro Tololo 0.9m and 1.5m reflector observations.
Tables 1-4: photoelectric sequence stars in the region of U Car, XZ Car, QY Cen, VX Cru, and AA Nor.
See also [VBA82], [VYB83], [TVY93]. Ref:=1985ApJS...57..743V byVAN DEN BERGH S. , YOUNGER P.F., TURNER D.G. Astrophys. J., Suppl. Ser., 57, 743-750 (1985) A search for OB associations near long-period Cepheids. III. U Carinae, XZ Carinae, QY Centauri, VX Crucis and AA Normae . oTable 1: <[VYT85] U Car A> (Nos A-H). Table 2: <[VYT85] XZ Car A> (Nos A-N). Table 3: <[VYT85] QY Cen A> (Nos A-N). Table 4: <[VYT85] VX Cru A> (Nos A-J). Table 5: <[VYT85] AA Nor A> (Nos A-J). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [VYW2001]
   [VYW2001] (Verdes-Montenegro+Yun+Williams+, 2001) (Not yet in Simbad) Write:<<[VYW2001] HCG NNT>> N: 9 Object:Tidal feature  (SIMBAD class: PartofG = Part of a Galaxy) Note:N=9 HCG groups present tidal features (tail, bridge,..) external to galaxies, but linked with the group. in source:HCG 2 in source:HCG 16 Originof the Acronym: S = Created by Simbad, the CDS Database in source:HCG 31 in source:HCG 49 in source:HCG 79 in source:HCG 88 in source:HCG 92 = Stephan's Quintet in source:HCG 95 in source:HCG 96 Ref:=2001A&A...377..812V byVERDES-MONTENEGRO L. , YUN M.S., WILLIAMS B.A., HUCHTMEIER W.K., DEL OLMO A., PEREA J. Astron. Astrophys., 377, 812-826 (2001) Where is the neutral atomic gas in Hickson groups? oTable 3: <[VYW 2001] HCG NNT> N=9.
Details on Acronym:   [VZA2004]
   [VZA2004] (Vivas+Zinn+Abad+, 2004) Write:<<[VZA2004] NNN>> N: 498 Object:RR Lyr  (SIMBAD class: RRLyr = Variable Star of RR Lyr type) Stat:is completely incorporated in Simbad Note:Survey of 380deg2 of the sky with the 1m Schmidt telescope of the Llano del Hato Observatory and the QUEST CCD camera: 498 RR Lyrae are identified. Ref:=2004AJ ....127.1158V byVIVAS A.K. , ZINN R., ABAD C., ANDREWS P., BAILYN C., BALTAY C., BONGIOVANNI A., BRICENO C., BRUZUAL G., COPPI P., DELLA PRUGNA F., ELLMAN N., FERRIN I., GEBHARD M., GIRARD T., HERNANDEZ J., HERRERA D., HONEYCUTT R., MAGRIS G., MUFSON S., MUSSER J., NARANJO O., RABINOWITZ D., RENGSTORF A., ROSENZWEIG P., SANCHEZ Ge., SANCHEZ Gu., SCHAEFER B., SCHENNER H., SNYDER J.A., SOFIA S., STOCK J., VAN ALTENA W., VICENTE B., VIEIRA K. Astron. J., 127, 1158-117 5 (2004) The QUEST RR Lyrae survey. I. The first catalog. oTable 2: <[VZA2004] NNN> (Nos 1-498). =E=Catalogue in electronic form as J/AJ/127/1158 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [VZG2008]
   [VZG2008] (Verdugo Ziegler+Gerken, 2008) Write:<<[VZG2008] rNNN-N JHHMMSS+DDMMSS>>
<<[VZG2008] Group N>>
<<[VZG2008] rNNNN-NNa>>
<<[VZG2008] ba-NN>>
<<[VZG2008] xdcNN-NN>> N: 286 Object:Group of G + G  (SIMBAD class: Galaxy) Note:Calar Alto 3.5m MOSCA spectroscopy of cluster galaxies. Ref:=2008A&A...486....9V byVERDUGO M. , ZIEGLER B.L., GERKEN B. Astron. Astrophys., 486, 9-24 (2008) The galaxy populations from the centers to the infall regions in z≃0.25 clusters. oTable 2, col(1): <[VZG2008] Group N> (Nos 1-4) = Table 2, col(2): <[VZG2008] rNNN-N JHHMMSS+DDMMSS> N=4. Table 3: <[VZG2008] rNNNN-NNa> N=274, <[VZG2008] ba-NN> N=12 among (Nos 07-39), <[VZG2008] xdc29-04> N=1. =E=Catalogue in electronic form as J/A+A/486/9 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [VZH2013]
   [VZH2013] (Vasquez+Zoccali+Hill+, 2013) Write:<<[VZH2013] JHHMMSS.ss+DDMMSS.s>> N: 450  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:ESO 2.2m telescope WFI photometry and Las Campanas Magellan IMACS and VLT FLAMES GIRAFFE spectroscopy of N=454 stars in the Milky Way bulge. in source:NAME Galactic Bulge Ref:=2013A&A...555A..91V byVASQUEZ S. , ZOCCALI M., HILL V., RENZINI A., GONZALEZ O.A., GARDNER E., DEBATTISTA V.P., ROBIN A.C., REJKUBA M., BAFFICO M., MONELLI M., MOTTA V., MINNITI D. Astron. Astrophys., 555A, 91-91 (2013) 3D kinematics through the X-shaped Milky Way bulge. obulge_rc: <[VZH2013] JHHMMSS.ss+DDMMSS.s> N=454. =E=Catalogue in electronic form as J/A+A/555/A91 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [VZH2015]
   [VZH2015] (Vasquez+Zoccali+Hill+, 2015) Write:<<[VZH2015] RGB NNNNNN>>
<<[VZH2015] RC NNNNNN>> N: 148 Object:* + RGB  (SIMBAD class: Star) Note:VLT FLAMES GIRAFFE spectroscopic observations of N=148 K giant stars in the Galactic bulge. in source:NAME Galactic Bulge Ref:=2015A&A...580A.121V byVASQUEZ S. , ZOCCALI M., HILL V., GONZALEZ O.A., SAVIANE I., REJKUBA M., BATTAGLIA G. Astron. Astrophys., 580A, 121-121 (2015) Calcium triplet metallicity calibration for stars in the Galactic bulge. oTable 2: <[VZH2015] RGB NNNNNN> N=68 among (Nos 44560-596502), <[VZH2015] RC NNNNNN> N=80 among (Nos 78195-575542). =E=Catalogue in electronic form as J/A+A/580/A121 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [VZK2001]
   [VZK2001] (Van Loon+Zijlstra+Kaper+, 2001) Write:<<[VZK2001] HS 327W>>
<<[VZK2001] A>>
<<[VZK2001] Carbon>>
<<[VZK2001] Red>> N: 2+3+1+1 Object:Cluster of * + *  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:Fig.2: [HS66] 327 is composed of 2 distinct stellar clusters: HS 327W and HS 327E. Tables 1, 2: N=3 brightest stars (Nos A-C), N=1 Carbon star, and N=1 Red star. in source:Magellanic Clouds:LMC:[HS66] 327 = [HS66] 327 Ref:=2001A&A...368..239V byVAN LOON J.T. , ZIJLSTRA A.A. Originof the Acronym: S = Created by Simbad, the CDS Database byKAPER L. , GILMORE G.F., LOUP C., BLOMMAERT J.A.D.L. Astron. Astrophys., 368, 239-249 (2001) The peculiar cluster HS 327 in the Large Magellanic Cloud: can OH/IR stars and carbon stars be twins? oStandard star S 121-E = GSPC S121-E oText: <[VZK2001] HS 327W> (Nos E, W). Tables 1, 2: <[VZK2001] A> (Nos A-C), <[VZK2001] Carbon> N=1, <[VZK2001] Red> N=1.
Details on Acronym:   [VZW98]
   [VZW98] (Van Loon+Zijlstra+Whitelock+, 1998) Write:<<[VZW98] NNN>> N: 3 among N>321 Object:OH-IR  (SIMBAD class: OH/IR = OH/IR star) Note:N=3 objects without known counterpart, fou nd in a survey of OH emission maser. Ref:=1998A&A...329..169V byVAN LOON J.T. , ZIJLSTRA A.A., WHITELOCK P.A., TE LINTEL HEKKERT P., CHAPMAN J.M., LOUP C., GROENEWEGEN M.A.T., WATERS L.B.F.M., TRAMS N.R. Astron. Astrophys., 329, 169-185 (1998) Obscured Asymptotic Giant Branch stars in the Magellanic Clouds. IV. Carbon stars and OH/IR stars. oFig.2: C* C4.5 = [VZK2001] Carbon in SIMBAD oTable 3: <[VZW98] NNN> N=3 among 321 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   W
   W (Window) ***** Avoid the usage of W, prefer [BBS2005] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Wackering) S ***** Avoid the usage of W, prefer CD Originof the Acronym: L (2001Ap&SS.275..441M)
Details on Acronym:   W
   W (Wilson)
Details on Acronym:   GCRV
   GCRV ***** Avoid the usage of GCRV, prefer GCRV
Details on Acronym:   W
   W (West) ***** Avoid the usage of W, prefer [GEO97] Originof the Acronym: L (1998ApJ...509..678G)
Details on Acronym:   W
   W (Woolley) ***** Avoid the usage of W, prefer GJ
Details on Acronym:   W
   W (Walter+) ***** Avoid the usage of W, prefer ScoPMS Originof the Acronym: L (1998A&A...332..825S)
Details on Acronym:   W
   W (Westerbork radio telescope) ***** Avoid the usage of W, prefer [TGC96] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Westerhout) Write:<<W NNa>>
<<W NNaNN>>
<<W NNW(OH)>>
<<W NN(H2O)>> 1e23 N: 82+? Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:(Nos 1-82).
Format NNa appears for the first times in 1969MNRAS.142..453W for W 49a and b, and in 1972MNRAS.157...31M, for W 51a to W 51h, W 51i is added in 1994ApJS...91..713M.
Format '51aN' appears for the first time in 1978MNRAS.183..435S. Ref:=1958BAN....14..215W byWESTERHOUT G. Bull. Astron. Inst. Netherlands, 14, 215-260 (1958) A survey of the continuous radiation from the galactic system at a frequency of 1390 Mc/s . o<W NNA> (Nos 1-82) Ref:=1969MNRAS.142..453W byWYNN-WILLIAMS C.G. Mon. Not. R. Astron. Soc., 142, 453-464 (1969) High resolution observations of the radio source W 49. o<W 49A> (Nos 49A, 49B). Ref:=1972MNRAS.157...31M byMARTIN A.H.M. Mon. Not. R. Astron. Soc., 157, 31-40 (1972) High resolution observations of W51. o<W 51A> (Nos W51A to W51H). Ref:=1978MNRAS.183..435S bySCOTT P.F. Mon. Not. R. Astron. Soc., 183, 435-442 (1978) High resolution radio observations of G49.5-0.4 ( W521). oauthors use minus letters: W 51e1 and e2 o<W51E1>, <W 51E2>. Ref:=1993ApJ...417..645G byGAUME R.A. , JOHNSTON K.J., WILSON T.L. Astrophys. J., 417, 645-654 (1993) High-resolution centimeter radio continuum and ammonia maser observation s of the W 51 region of star formation. oauthors use minus letters: W 51dN and W 51eN o<W 51D1>, <W 51D2>, <W 51E3>, <W 51E4>, <W 51E5> Ref:=1994ApJS...91..713M byMEHRINGER D.M. Astrophys. J., Suppl. Ser., 91, 713-748 (1994) Radio continuum and radio recombination line observations of W 51. oTable 2: <[M94] LL.l-B.bb> N=9, and <[M94] LL.l-B.b aN> N=22. <[M94] 49.5-0.4 aN> = W 51AN (Nos W 51E6, W 51E7, W 51I) are new Ref:=1997ApJ...488..241Z byZHANG Q. , HO P.T.P. Astrophys. J., 488, 241-257 (1997) Dynamical collapse in W51 massive cores: NH_{3} observations. Originof the Acronym: A = Assigned by the author(s) oW 51e8 = W 51E8 o<W 51E8> Auth.:ZHANG Q.+ Ref:=2016A&A...595A..27G byGINSBURG A. , GOSS W.M., GODDI C., GALVAN-MADRID R., DALE J.E., BALLY J., BATTERSBY C.D., YOUNGBLOOD A., SANKRIT R., SMITH R., DARLING J., KRUIJSSEN J.M.D., LIU H.B. Astron. Astrophys., 595A, 27-27 (2016) Toward gas exhaustion in the W51 high-mass protoclusters. oFig. 2, Table 3: <W51aNN> (Nos W51d3-d7, W51e9-e23) added. Figs 2+A.2, Tables 3-8: <[GGG2016] arc> N=1, <[GGG2016] W51aNNw> (Nos 1.0 - 10-Jan-2012 - Ajout e-version: J/A+A/493/79/
Details on Acronym:   Cl* Alicante 5 MN
   Cl* Alicante 5 MN E Marco + Negueruela Write:<<Cl* Alicante 5 MN NNN>> N: 105 Object:*inCl Ref:=2009A&A...493...79M byMARCO A. , NEGUERUELA I. Astron. Astrophys., 493, 79-88 (2009) The open cluster Pismis 11 and the very luminous blue supergiant HD 80077. I. Physical parameters of the cluster. oParagr.2.2: .
Details on Acronym:   Cl* Basel 13 H
   Cl* Basel 13 H (Hassan) Write:<<Cl* Basel 13 H NNN>> N: 77 Object:*inCl Ref:=1975A&AS...20..255H byHASSAN S.M. Astron. Astrophys., Suppl. Ser., 20, 255-267 (1975) The stellar groups Ba12, Ba13, Ba14 and Ba15. oTable 1: <Cl* Basel 12 H NN> (Nos 1-75), <Cl* Basel 13 H NNN> N=77 among (Nos 1-100), <Cl* Basel 14 H NNN> (Nos 1-107), <Cl* Basel 15 H NNN> (Nos 1-117). 02.12.02
Details on Acronym:   Cl* Basel 14 DAF
   Cl* Basel 14 DAF (Dias+Assafin+Florio+) Write:<<Cl* Basel 14 DAF NNN>> N: 238 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 d variables - VII. Berkeley 58 and CG Cassiopeiae. oTable 1: <Cl* Berkeley 58 TFE NN> (Nos 1-37). Table 3: <Cl* Berkeley 58 TFE NNN> (Nos 101-255). Table 4: <Cl* Berkeley 58 TFE NNNN> (Nos 1001-1411). =E=Catalogue in electronic form as <J/MNRAS/388/444/>
Details on Acronym:   Cl* Berkeley 59 PSO
   Cl* Berkeley 59 PSO (Pandey+Sharma+Ogura+) Write:<<Cl* Berkeley 59 PSO NNNN>> N: 5944 Object:*inCl Ref:=2008MNRAS.383.1241P .299....1S bySAGAR R. , GRIFFITHS W.K. Mon. Not. R. BAYASHI H., KURABAYASHI T., NAKAI T., HYAKKAI M., ARIMOTO N. Publ. Astron. Soc. Jap., 56, 295-311 (2004) New p lorio+ Write:<<Cl* Bochum 9 DAF NNN>> N: 605 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. oC VRI observations of stars in the fields of five open clusters with nearby carbon stars. oTable II: <Cl* NGC 2533 JW NN> (Nos 1-17), <Cl* Haffner 14 JW NN> (Nos 1-25), <Cl* IC 2395 JW NN> (Nos 1-14), <Cl* Lynga 2 JW NN> (Nos 1-27). Table II: Cl* Loden 1409 JW NN> (Nos 1-36).
Details on Acronym:   Cl* IC 2395 L
   Cl* IC 2395 L (Lynga) **
Details on Acronym:   IC 4756
   IC 4756 Write:<<IC 4756 NNN>> N: 203 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1943AN....274...69K byKOPFF E. Astron. Nachr., 274 IBERO 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>. =E=Catalogue in electronic form as <J/A+A/446/949/>
Details on Acronym:   Cl* Kharchenko 3 DAF
   Cl* Kharchenko 3 DAF (Dias+Assafin+Florio+) Write:<<Cl* Kharchenko 3 DAF NNN>> N: 121 Object:*inCl Ref:=2006A&A...446..949D 7 HJI (Hoag+Johnson+Iriarte+) ====>Equivalent to: NGC 1027
Details on Acronym:   Cl* NGC 1027 Hoag
   Cl* NGC 1027 Hoag (Hoag+) ====>Equivalent to: NGC 1027
Details on Acronym:   Cl* NGC 1027 MMU
   Cl* NGC 1027 MMU (Mermillod+Mayor+Udry) Write:<<Cl* NGC 1027 MMU NN>> N: 3 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. canae. oV101 in M 5 = Cl* NGC 5904 SAW V101 o<Cl* NGC 104 PD VN> (N
Details on Acronym:   Cl* NGC 1466 P
   Cl* NGC 1466 P Write:<<Cl* NGC 1466 P A>> N: 10 Object:*inCl Ref:=1981MNRAS.197..693P byPENNY A.J. Mon. Not. R. Astron. Soc., 197, 693-698 (1981) Three UBV sequences in the LMC. o<Cl* NGC 1466 P A> (Nos A-H, M, P), <Cl* NGC 2214 P A> (Nos A-D, F, G), <Cl* NGC 2257 P A> (Nos A, B, E-N, P, Q), <Cl* NGC 2257 P AA> (Nos AA, AB, KK>
Details on Acronym:   Cl* NGC 1851 Alc
   Cl* NGC 1851 Alc (Alcaino) ====>Equivalent to: NGC 1851
Details on Acronym:   Cl* NGC 1851 Alc
   Cl* NGC 1851 Alc (Alcaino) Write:<<Cl* NGC 1851 Alc NNN>> N: 127 Object:*inCl Ref:=1976A&A....50..299A byALCAINO G. Astron. Astrophys., 50, 299-303 (1976) The X-ray globular cluster NGC 1851. oTable 2: <Cl* NGC 1851 Alc NNN> (Nos 1-127).
Details on Acronym:   Cl* NGC 1851 BPF
   Cl* NGC 1851 BPF (Bellazini+Pecci+F) ). Auth.:BELLAZZINI M.+ =E=Catalogue in electronic form as <J/AJ/122/2569/>
Details on Acronym:   Cl* NGC 1851 DA
   Cl* NGC 1851 DA (Da Costa+Armandroff) 8.10 Auth.:PURGATHOFER A.
Details on Acronym:   Cl* NGC 1866 AM
   Cl* NGC 1866 AM (Aaronson+Mould) Write:<<Cl* NGC 1866 AM N>> N: 3 among 4 Object:*inCl Ref:=1985ApJ...288..551A byAARONSON M. , MOULD J. Astrophys. J., 288, 551-557 (1985) The extended giant branches of intermediate age globular clusters in the Magellanic Clouds. IV. oTable 1: <Cl* Lindsay 44 AM N> (No. 1), <Cl* Lindsay 47 AM N> (Nos 1-3), <Cl* Lindsay 53 AM N> (No. 1), <Cl* Lindsay 114 AM N> (Nos1-3), <Cl* NGC 1856 AM N> ared study of NGC 2024. o<NGC 2024 N> (No. 2) added. C 2214 MTP N> (No. 1), <Cl* NGC 2107 MTP N> (No. 1).
Details on Acronym:   Cl* NGC 2214 P
   Cl* NGC 2214 P (Penny) Write:<<Cl* NGC 2214 P A>> N: 6 Object:*inCl Ref:=1981MNRAS.197..693P byPENNY A.J. Mon. Not. R. Astron. Soc., 197, 693-698 (1981) Three UBV sequences in the LMC. o<Cl* NGC 1466 P A> (Nos A-H, M, P), <Cl* NGC 2214 P A> (Nos A-D, F, G), <Cl* NGC 2 , No. 32, p. 7) oTable 3: <Cl* AAAAA NNNN MMU NNNNN> N=1260 in N=187 clusters. (AAAAA = cluster name). =E=Catalogue in electronic form as <J/A+A/485/303/>
Details on Acronym:   Cl* NGC 225 RH
   Cl* NGC 225 RH (Rose+Hintz) Write:<<Cl* NGC 225 RH NNN>> N: 21 Object:*inCl Ref:=2007AJ....134.2067R byROSE M.B. , HINTZ E.G. Astron. J., 134, 2067-2078 (2007) A search for low-amplitude variability in six open clusters using th r
Details on Acronym:   Cl* NGC 2264 J
   Cl* NGC 2264 J (Jones) s 1-274), <Cl* NGC 2437 AR NNN> (Nos 1-278), <Cl* NGC 2451 AR NNN> (Nos Society, No. 32, p. 7) oTable 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:   Cl* NGC 2439 PM
   Cl* NGC 2439 PM (Paunzen+Maitzen) Write:<<Cl* NGC 2439 PM NNN>> N: 113 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for pecu ocities. oCatalog: <Cl* NGC 2682 YBP NNNN> (Nos 1-2410). =E=Catalogue in electronic form as <J/A+A/484/609/>
Details on Acronym:   Cl* NGC 2682 ZTP
   Cl* NGC 2682 ZTP (Zhao+Tian+Pan+) Write:<<Cl* NGC 2682 ZTP NNNN>> N: 1046 Object:*inCl Ref:=1993A&AS..100..243Z byZHAO J.L. , TIAN K.P., PAN R.-S., HE Y.P., SHI H.M. Astron. Astrophys., Suppl. Ser., 100, 243-261 (1993) Study of proper motions in the region of the open cluster M67 and membership of stars. oTable 6: <CL* NGC 2682 ZTP NNNN> N= 1046 among (Nos 1-1067).
Details on Acronym:   Cl* NGC 269 FMB
   Cl* NGC 269 FMB iller
Details on Acronym:   Cl* NGC 339 AAWL
   Cl* NGC 339 AAWL Write:<<Cl* NGC 339 AAWL A>> N: 4 Object:*inCl Ref:=1990AJ.....99.1488A byALCAINO G. , ALVARADO F., WENDEROTH E., LILLER W. Astron. J., 99, 1488-1490 (1990) Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466. oTable III: <Cl* Lindsay 1 AAWL A> (Nos A-K). Table IV: <Cl* NGC 339 AAWL A> (Nos A-D). Table V: <Cl* NGC 361 AAWL A> (Nos A-F). Table VI: <Cl* NGC 1466 AAWL A> (Nos A-G).
Details on Acronym:   Cl* NGC 339 FMB
   Cl* NGC 339 FMB (Frogel+Mould+Blanco) Write:<<Cl* NGC 339 FMB N>> N: 7 Object:*inCl Ref:=1990ApJ...352...96F byFROGEL J.A. , MOULD J., BLANCO V.M. Astrophys. J., 352, 96-122 (1990) The asymptotic giant branch of Magellanic Cloud clusters. oin ref list BLANCO 1987AJ.....93..321B instead of AJ.92, MOULD J., REID N. 1987ApJ...321..156M instead of ApJ.321.156. Finding charts kindly provide d by J.A. Frogel (no coordinates in the article); cross-identifications in the SMC perfo ntermediate-age open cluster NGC 3960. oTable 3, col.(2): <Cl* NGC 3960 BT, NOBLE R.G., DICKENS R.J., BUTTRESS J., G 95 (1983) Photoeletric photometry of globular cluster giants. oonly the clusters are in SIMBAD, not the stars. o<Cl* NGC 5904 TLE 1>
Details on Acronym:   Cl* NGC 5904 VFP
   Cl* NGC 5904 VFP (Valenti+Ferraro+Perina+) Write:<<Cl* NGC 5904 VFP NNN>> N: 882 Object:*inCl Ref:=2004A&A...419..139V byVALENTI E. , FERRARO F.R., PERINA S., ORIGLIA L. Astron. Astrophys., 419, 139-147 (2004) Near-IR photometry of five Galactic Globular Clusters. om3.dat: <Cl* NGC 5272 VFP NNNN> (Nos 1-1414). m5.dat: <Cl* NGC 6254 VFP NNN> ( Cl Ref:=1999ApJ...522..983F byFERRARO F.R. , PALTRINIERI B., ROOD R.T., DORMAN B. Astrophys. J., 522, 983-990 (1999) Blue straggler stars: the spectacular population in M80. oTable 1, col(1): <Cl* NGC 6093 BSS NNN> (Nos 1-305) = Table 1, col(2): <Cl* NGC 6093 FPR NNNNN> N=305 among 13000. Table 2, col(1): <Cl* NGC 6093 EBSS NN> (Nos 1-19) = Table 2, col(2): <Cl* NGC 6093 FPR NNNNN> N=19 among 13000.
Details on Acronym:   Cl* NGC 6093 HR
   Cl* NGC 6093 HR (Harris+Racine) Write:<<Cl* NGC 6093 HR I-NNN>>
<<Cl* NGC 6093 HR II-NN>> N: 286+82 d on the UCAC2 catalogue. oCatalogs pm: <Cl* AAAAAA NNNN DAF NNNN>. Auth.:DIAS W.S.+ =E=Catalogue in electronic form as <J/A+A/446/949/>
Details on Acronym:   Cl* NGC 6193 HG
   Cl* NGC 6193 HG (Huang+Gies) Write:<<Cl* NGC 6193 HG NNNNN # always 5 digits>> N: 20 Object:*inCl Ref:=2006ApJ...648..580H byHUANG W. , GIES D.R. Astrophys. J., 648, 580-590 (2006) Stellar rotation in young clusters. I. Evolution of projected rotational velocity distributions. oTable 3: <Cl* IC 2944 HG NNNNN> N=5 among (Nos 10002-10012), <Cl* NGC 2362 HG NNNNN> (Nos 10005-10011), <Cl* NGC 2384 HG NNNNN> (Nos 10020-10032), <Cl* NGC 2467 HG NNNNN> (No. 10017), <Cl* NGC 4755 HG NNNNN> N=3 among (Nos 10046-10238), <Cl* Trumpler 14 HG NNNNN> (Nos 10040-10041), <Cl* Trumpler 16 HG NNNNN> (Nos 10047-10048). 6 07.03.18 =E=Catalogue in electronic form as <J/ApJ/648/580/>
Details on Acronym:   Cl* NGC 6193 HH
   Cl* NGC 6193 HH (Herbst+H) avlen ====>Equivalent to: [HH77]
Details on Acronym:   Cl* NGC 6193 MG
   Cl* NGC 6193 MG (McSwain+Gies) A KALUZNY J. Astron. Astrophys., Suppl. Ser., 122, 1-7 (1997) CCD photometry of variable stars in the field of the globular cluster NGC 6397. oTable 2: <Cl* NGC 6397 SAW VNN> (Nos V4-V11) added. Tables 5-6: <Cl* NGC 6397 K NNNNN> (Nos 1-17559). Auth.:KALUZNY J. Ref:=2003AJ....125.2534K byKALUZNY J. , THOMPSON I.B. Astron. J., 125, 2534-2542 (2003) Time series photometry R T., TOMASELLA L. Astron. Astrophys., Suppl. Ser., 144, 451-456 (2000) 57+? Object:*inCl Rem:Format 'NN' for photoelectrically measured stars.
Format te dwarfs. oTable 2: <Cl* NGC 6791 KBH NN> (Nos 1-14).
Details on Acronym:   Cl* NGC 6791 Kin
   Cl* NGC 6791 Kin (Kinman) ====>Equivalent to: NGC 6791
Details on Acronym:   Cl* NGC 6791 Kin
   Cl* NGC 6791 Kin (Kinman) Write:<<Cl* NGC 6791 Kin A>>
<<Cl* NGC 6791 Kin a>> N: 25+13 Object:*inCl Ref:=1965ApJ...142..655K byKINMAN T.D. Astrophys. J., 142, outlying blue horizontal-branch stars in globular clusters. oTable 2: <Cl* NGC 288 San NN> 'ONN' for outside stars. Ref:=1961TrPul..73....5L byLAVDOVSKY V.V. Tr. Glav. Astron. Obs. Pulkovo, ser. 2, 73, 5-131 (1961) A catalogue of proper motions of stars in 13 open clusters and in their vicinity. oTables 1-2, 8-11: <Cl* NGC NNNN LAV NNNN>, <Cl* NGC NNNN LAV ONN>. Table 5: <Cl* NGC 869 LAV NNNN> (Nos 1-1389), <Cl* NGC 884 LAV NNNN> (Nos 1374-2565). Tables 6-7: <Cl* NGC 1912 LAV 6-NNNN>, <Cl* NGC 1912 , 90, 31-82 (1994) Young open clusters as probes of the star formation process. I. An atlas of open cluster photometry. oThe stars in each cluster and their numbering are not published, but they are used in literature. oFrom Table 4: <Cl* Berkeley 7 PJ NNN> (Nos 1-723), <Cl* NGC 663 PJ NNNN> (Nos 1-3012), <Cl* NGC 659 PJ NNN> (Nos 1-637), <Cl* NGC 654 PJ NNN> (Nos 1-582 N: 55 Object:*inCl Ref:=2006ApJ...648..580H byHUANG W. , GIES D.R. Astrophys. J., 648, 580-590 (2006) Stellar rotation in young clusters. I. Evolution of projected rotational velocity distributions. oTable 3: <Cl* IC 2944 HG NNNNN> N=5 among (Nos 10002-10012), <Cl* NGC 2362 HG NNNNN> (Nos 10005-10011), <Cl* NGC 2384 HG NNNNN> (Nos 10020-10032), <Cl* NGC 2 PJM NNNN> Nos among (Nos 1-2235), <Cl* King 5 PJM NNNN> Nos among (Nos 1-1347), <Cl*Ki Table 1: <Cl Pismis 5 N> (Nos 1-9). Table 2: <Cl Collinder 197 NN> (Nos 1-22) No 12 missing. Table (Nos 1-3) are in Sh 2-208, see MFJ. Ref:=1979A&AS...38..197M byMOFFAT A.F.J. , FITZGERALD M.P., JACKSON P.D. Astron. Astrophys., Suppl. Ser., 38, 197-225 (1979) The rotation and structure of the galaxy beyond the solar circle. I. Photometry and spectroscopy of 276 stars in 45 HII regions and other young stellar groups toward the galactic anticentre. oStars in SH 2-305 are '[VM75] SH 2-NN', Stars in SH 2-253 and in RCW 19 are 'LS NNNN', Stars in SH 2-284 = Dolidze 25 are 'Cl* Dolidze 25 MV NN' oTable 1: <Cl Waterloo N> (Nos 1-3). Table 1: <MFJ SH 2-NNN NNW> N=212, <MFJ RCW 20 N> (Nos 1-7). Table 1: <Cl* Waterloo 1 MFJ NN> (Nos 4-12), <Cl* Waterloo 2 MFJ NN> (Nos 5-10), <Cl Waterloo 3 N> (Nos 1-7), <Cl* Dolidze 24 MFJ N> (Nos 1-8), <Cl* Bochum 2 MFJ N> (Nos 1-3). Auth.:MOFFAT A.F.J.+
Details on Acronym:   Cl* Waterloo 2 MFJ
   Cl* Waterloo 2 MFJ (Moffat+Fitzgerald+Jackson) Write:<<Cl* Waterloo 2 MFJ NN>> N: 6 Object:*inCl Rem:Only (Nos 5-10) are in Wat 2, named 'Cl* Waterloo 2 MFJ NN',
(Nos 1-4, 11, 12) are in Sh 2-225, see MFJ. Ref:=1979A&AS...38..197M byMOFFAT A.F.J. , FITZGERALD M.P., JACKSON P.D. Astron. Astrophys., Suppl. Ser., 38, 197-225 (1979) The rotation and structure of the galaxy beyond the solar circle. I. Photometr

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