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

Result of query: info cati HH$
 .
oTable 2: <[HGP92] NGC NNNN HHMMSS.ss+DDMMSS.s> and <[HGP92] PAL NN    HHMMSS.ss+DDMMSS.s> N=130
 Auth.:HARRIS H.C.+

Details on Acronym:   [HGR2010]
   [HGR2010] (Held+Gullieuszik+Rizzi+, 2010) Write:<<[HGR2010] NNNNNN>> N: 7471 Object:*  (SIMBAD class: Star) Note:UKIRT WFCAM observations of the dwarf spheroidal galaxy Leo I. in source:UGC 5470 = Leo I Ref:=2010MNRA S.404.1475H byHELD E.V. , GULLIEUSZIK M., RIZZI L., GIRARDI L., MARIGO P., SAVIANE I. Mon. Not. R. Astron. Soc., 404, 1475-1489 (2010) A near-infrared study of AGB and red giant stars in the Leo I dSph galaxy. oTable 2: <[HGR2010] NNNNNN> N=7471 among (Nos 41-200324). =E=Catalogue in electronic form as J/MNRAS/404/1475 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [HGS97]
   [HGS97] (Hammer+Gioia+Shaya+, 1997) (Not yet in Simbad) Write:<<[HGS97] SN>>
<<[HGS97] A>> N: 3+5 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Note:HST WFPC2 images of the cluster of galaxies 1E 2137.3-2353.
Fig.5: sources (Nos S1-S3): Sources of arc images in [FLH92].
Fig.5: 5 knots (Nos A-E). in source:1E 2137.0-2353 Ref:=1997ApJ...491..477H byHAMMER F. , GIOIA I.M., SHAYA E.J., TEYSSANDIER P., LE FEVRE O., LUPPINO G.A. Astrophys. J., 491, 477-482 (1997) Detailed lensing properties of the MS 2137-2353 core and reconstruction of sources from Hubble Space Telescope imagery. oFig.2: <[FLH92] AR> N=1 added, <[FLH92] ARN> N=1 added, <[FLH92] A01 SKN> (Nos SK1-SK2) added, <[FLH92] A02 SKN> (Nos SK1-SK2) added. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   HGT
   HGT (Halpern+Grindlay+Tytler) Write:<<HGT NNN>> N: 61+76 Object:*  (SIMBAD class: Star) Note:(Nos 1-61) in the first ref., (Nos 101-176) in the second ref. Identif. charts Ref:=1985ApJ...296..190H byHALPERN J.P. , GRINDLAY J.E., TYTLER D. Astrophys. J., 296, 190-196 (1985) Observations of the Geminga optical candidate. o<HGT NN> (Nos 1-61) Ref:=1988ApJ...330..201H byHALPERN J.P. , TYTLER D. Astrophys. J., 330, 201-217 (1988) The Geminga X-ray counterpart and a blue optical identification. o<HGT NNN> (Nos 101-176) Originof the Acronym: L = Found in the literature
Details on Acronym:   [HGT2015]
   [HGT2015] (Ho+Geha+Tollerud+, 2015) Write:<<[HGT2015] M32 NN>>
<<[HGT2015] NGC205 NNN>>
<<[HGT2015] NGC185 NNN>>
<<[HGT2015] NGC147 NNN>>
<<[HGT2015] AndVII NNN>>
<<[HGT2015] AndII NNN>> 300 N: 1243 Object:RGB*  (SIMBAD class: RGB* = Red Giant Branch star) Stat:is completely incorporated in Simbad Note:Keck II DEIMOS observations of N=64+224+321+230+104+300 red giant branch member stars for the six most luminous M31 dwarf galaxy satellites: M32, NGC 205, NGC 185, NGC 147, Andromeda VII and Andromeda II. Ref:=2015ApJ...798...77H byHO N. , GEHA M., TOLLERUD E.J., ZINN R., GUHATHAKURTA P., VARGAS L.C. Astrophys. J., 798, 77 (2015) Metallicity evolution of the six most luminous M31 dwarf satellites. oTable 2: <[HGT2015] M32 NN> (Nos 1-64), <[HGT2015] NGC205 NNN> (Nos 1-224), <[HGT2015] NGC185 NNN> (Nos 1-321), <[HGT2015] NGC147 NNN> (Nos 1-230), <[HGT2015] AndVII NNN> (Nos 1-104), <[HGT2015] AndII NNN> (Nos 1-300). =E=Catalogue in electronic form as J/ApJ/79 .06 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   OH
   OH (Olszewski+Harris+) ***** Avoid the usage of OH, prefer OHSC Originof the Acronym: L = Found in the literature
Details on Acronym:   OH1720
   OH1720 KWS Write:<<Cl* NGC 104 KWS N>> Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 104 BSS
   Cl* NGC 104 BSS (Blue Straggler Star) ====>Equivalent to: Cl* NGC 104 PSM
Details on Acronym:   Cl* NGC 104 Can
   Cl* NGC 104 Can (Cannon) Write:<<Cl* NGC 104 Can NN>> N: 22 Object:*inCl Ref:=1981MNRAS.195....1C byCANNON R.D. Mon. Not. R. Astron. Soc., 195, 1-13 (1981) Photometry of southern globular clusters. IV. Faint photoelectric sequences i
Details on Acronym:   Cl* NGC 1806 FFT
   Cl* NGC 1806 FFT (Ferraro+Fusi Pecci+Testa+) Write:<<Cl* NGC 1806 FFT NN>> N: 70 Object:*inCl Stat:is completely incorporated in Simbad Ref:=1995MNRAS.272..391F byFERRARO F.R. , FUSI PECCI F., TESTA V., GREGGIO L., CORSI C.E., BUONANNO R., TERNDRUP D.M., ZINNECKER H. Mon. Not. R. Astron. Soc., 272, 391-422 (1995) Globular clusters in the Magellanic Clouds - II. IR-array photometry for 12 globular clusters and contributions to the integrated cluster light. Write:<<Cl* NGC 2632 WSPH AN>> N: 3 Object:*inCl Ref:=1994PASP..106..817W 448 byWILLIAMS S.D. , STAUFFER J.R., PROSEER C.F., HERTER T. Publ. Astron. Soc. Pac., 106, 817-821 (1994) Spectroscopy and photometry for low-mass stars in Praesepe. o<Cl* NGC 2632 WSPH AN> (Nos A1-A3)
Details on Acronym:   NGC 2635
   NGC 2635 Write:<<NGC 2635 N>> N: 6 Object:*inCl Ref:=1972A&AS....7..133V byVOGT N. , MOFFAT A.F.J. Astron. Astrophys., Suppl. Ser., 7, 133-167 (1972) Southern open star clusters. I. UVB-H β photometry of 15 clusters between galactic longitudes 231 ° and °. oTable 2: <NGC 2414 NN> (Nos 1-11). Table 3: <NGC 2383 NN> (Nos 1-11). Table 4: <NGC 2384 NN> (Nos (1-15). Table 5: <NGC 2367 NN> (Nos 1-15). Table 6: <Cl Tr ), <Cl* NGC 457 PJ NNNN> (Nos 1-3503), <Cl* NGC 436 PJ NNN> (Nos 1-891), <Cl* NGC 433 PJ NNNN> (Nos 1-2119), <Cl* NGC 381 PJ NNNN> (Nos 1-2254), <Cl* NGC 366 PJ NNNN> (Nos 1-1014), <Cl* Berkeley 62 PJ NNNN> (Nos 1-1572), <Cl* Czernik 2 PJ NNNN> (Nos 1-2337), <Cl* Stock 24 PJ NNNN> (Nos 1-2121), <Cl* NGC 146 PJ NNN> (Nos 1-620), <Cl* King 15 PJ NNNN> (Nos 1-1936), <Cl* NGC 129 PJ NNNN> (Nos 1-1158), <Cl* NGC 103 PJ NNNN> (Nos 1-2807), <Cl* G NNNN> (Nos 1-1188), <Cl* Hogg NN MG NNN> N=352+26, <Cl* IC NNNN MG NNN> N=180 N=1260 in N=187 clusters. (AAAAA = cluster name). =E=Catalogue in electronic form as <J> d of the format is a sector of a ring,
and the 3 last digits 'NNN' are the numbering of a star in each sector.
ex. star 39 in IV-1-B = Cl* NGC 6341 SK 41039B. Ref:=1983AJ.....88.1146S bySANDAGE A. , KATEM B. Astron. J., 88, 1146-1158 (1983) On the intrinsic width and luminosity function of the M 92 main sequence. oTables 1, 3: <Cl* NGC 6341 SK NNNNNA> N about 375.
Details on Acronym:   Cl* NGC 6341 SW
   Cl* NGC 6341 SW (Sandage+Walker) ====>Equivalent to: NGC 6341
Details on Acronym:   Cl*
   Cl* O G. byKING 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-magnitude diagrams of 74 galactic globular clusters in the HST F439W and F555W bands. oSee also authors database: http://dipastro.pd.astro.it/globulars 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+> 16 =E=Catalogue in electronic form as <J/MNRAS/382/1203/>
Details on Acronym:   Cl* NGC 6440 KF
   Cl* NGC 6440 KF (Kuchinski+Fr) ogel Write:<<Cl* NGC 6440 KF NN>> N: 97 Object:*inCl Ref:=1995AJ....110.2844K byKUCHINSKI L.E. , FROGEL J.A. Astron. J., 110, 2844-2861 (1995) Infrared array photometry of metal-rich globular clusters. III. Two more clusters and an analysis of V-K colors. oTable 2: <Cl* NGC 6624 KF NNN> (Nos 1-153), Table 3: <Cl* NGC 6440 KF NN> (Nos 1-97) =E=Catalogue in electronic form as <J/AJ/110/2844/>
Details on Acronym:   Cl* NGC 6440 Klem
   Cl* NGC 6440 Klem (Klemola) Write:<<Cl* NGC 6440 Klem >> tal-rich galactic globular clusters. oTable 2: <CL* NGC 104 SN NN> N=65. Table 3: <CL* NGC 5927 SN NNN> N=371. Table 4: <CL* NGC 6352 SN NNN> N=231. Table 5: <CL* NGC 6496 SN NNN> N=252. Table 6: <CL* NGC 6624 SN NNN> N=374. Table 7: <CL* NGC 6637 SN NNN> N=408 Auth.:SARAJEDINI A.+
Details on Acronym:   Cl* NGC 6624 SZR
   Cl* NGC 6624 SZR (Shara+Zurek+Ri) Appendix, added later in literature Ref:=1961PUSNO..17..343H byHOAG A.A. , JOHNSON H.L., IRIA IOTTO 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-magnitude diagrams of 74 galactic globular clusters in the HST F439W and F555W bands. oSee also authors database: http://dipastro.pd.astro.it/globulars or http://menhir.pd.astro.it o<Cl* NGC NNNN PKD NNNNN>, <Cl* IC NNNN PKD NNNNN>, for N=74 Cl* K., WILLEMSEN P.G. Astron. Astrophys., 486, 437-452 (2008) Comparing CN and CH line strengths in a homogeneous spectroscopic sample of 8 Galactic globular clusters. oTable 3 NGC 6839 is a probable misprint for NGC 6838. oTable A1: <Cl* NGC 288 KHG NN> (Nos 1-99), <Cl* NGC 362 KHG NN> (Nos 1-77), <Cl* NGC 5286 KHG NN> (Nos 1-10), <Cl* NGC 6656 KHG NN> (No

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