Dictionary of Nomenclature of Celestial Objects
(Last update: 11-Aug-2017)

Result of query: info cati WD$

Details on Acronym:   WD
   WD (Davis+Richer+Rich+, 2009) (Not yet in Simbad) ***** Avoid the usage of WD, prefer [DRR2009] Originof the Acronym: A (2009ApJ...705..408K)
Details on Acronym:   Wd
   Wd (Westerlund) (Not yet in Simbad) ***** Avoid the usage of Wd, prefer [W69c] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Wd
   Wd (Westerlund) ***** Avoid the usage of Wd, prefer Westerlund
Details on Acronym:   WD
   WD (cloud complex labelled WD) ***** Avoid the usage of WD, prefer [H68]
Details on Acronym:   WD
   WD (White Dwarf) ***** Avoid the usage of WD, prefer [KW2001b] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   WD
   WD (White Dwarf) ***** Avoid the usage of WD, prefer [NCA2002] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Wd
   Wd (Westerlund) ***** Avoid the usage of Wd, prefer [W60] Originof the Acronym: L = Found in the literature
Details on Acronym:   WD
   WD (White Dwarf) Write:<<WD HHMM+DD>>
<<WD HHMM+DDd>>
<<WD HHMM+DDdA>>
<<WD HHMM+DDda>>
<<WD HHMM+DDd.N>>
<<WD HHMM+DDdNN>> N: about 14000 Object:WD  (SIMBAD class: WD* = White Dwarf) Note:"A catalogue of spectroscopically identified white dwarfs."
Each version supersedes the precedent edition.
The formats 'HHMM+DDd.N' and 'HHMM+DDdNN' are used to distinguish stars having identical format 'HHMM+DDd'.
A version of the White Dwarf Catalog is available online at: http://www.astronomy.villanova.edu/WDCatalog/ Ref:=1977VilCo...2....0C byCOOK G.P. , SION E.M. Villanova Univ. Obs. Contr., 2, 0 (1977) A catalogue of spectroscopically identified white dwarfs. o<WD HHMM+DDA> N=528 Ref:=1984VilCo...3....1M byMcCOOK G.P. , SION E.M. Villanova Univ. Obs. Contr., 3, 1-120 (1984) A catalogue of spectroscopically identified white dwarfs. o<WD HHMM+DDdA> N about 1500 Ref:=1987ApJS...65..603M byMcCOOK G.P. , SION E.M. Astrophys. J., Suppl. Ser., 65, 603-671 (1987) A catalog of spectroscopically identified white dwarfs. oG 124-209 misprint for G 124-20 oTable 2: <WD HHMM+DDdA> N=1279 Ref:=1999ApJS..121....1M byMcCOOK G.P. , SION E.M. Astrophys. J., Suppl. Ser., 121, 1-130 (1999) A catalog of spectroscopically identified white dwarfs. oWD 2226+210 is a misprint for WD 2226-210 oTable 3: <WD HHMM+DDdA> N=2249. =E=Catalogue in electronic form as III/235 =E=Catalogue in electronic form as <III/235B/> =E=Catalogue in electronic form as <III/129/> =E=Catalogue in electronic form as <B/wd/> Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   WD
   WD (White Dwarf) ***** Avoid the usage of WD, prefer WOCS Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 104 FDP
   Cl* NGC 104 FDP (Ferraro+D'Amico+Possenti+) ====>Equivalent to: Cl* NGC 104 WD
Details on Acronym:   Cl* NGC 104 WD
   Cl* NGC 104 WD (White Dwarf *) Write:<<Cl* NGC 104 WD NN>> N: 12 Object:*inCl Ref:=2001ApJ...561..337F byFERRARO F.R. , D'AMICO N., POSSENTI A., MIGNANI R.P., PALTRINIERI B. Astrophys. J., 561, 337-345 (2001) Blue stragglers, young white dwarfs, and UV-excess stars in the core of 47 Tucanae. oTable 5: 'WNNN' = [GHE2001] WNNN. oTable 2, col(1): <Cl* NGC 104 PSM NN> (Nos 22-46) added. Tables 2 to 5, (col(2): <Cl* NGC 104 FDP NNNN> N=86 among about 4000. Table 3, col(1): <Cl* NGC 104 WD NN> (Nos 1-12). Table 4, col(1): <Cl* NGC 104 UVE NN> (Nos 1-11). Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 1261 WD
   Cl* NGC 1261 WD (Wehlau+Demers) ====>Equivalent to: Cl* NGC 1261 Saw
Details on Acronym:   Cl* NGC 188 WD
   Cl* NGC 188 WD (White Dwarf) ====>Equivalent to: Cl* NGC 188 VS Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 2099 WD
   Cl* NGC 2099 WD (White Dwarf) ====>Equivalent to: Cl* NGC 2099 KRR
Details on Acronym:   Cl* NGC 2420 WD
   Cl* NGC 2420 WD (White Dwarf) ====>Equivalent to: Cl* NGC 2420 VGWD Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 6791 WD
   Cl* NGC 6791 WD (White Dwarf) ====>Equivalent to: Cl* NGC 6791 KBH Originof the Acronym: A = Assigned by the author(s)

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