Details on Acronym: WD
WD (Position of a white dwarf in J2000 coordinates)
>>>>>> New acronym being registered Ref:=2019MNRAS.482.4570G byGENTILE FUSILLO N.P. , TREMBLAY P.-E., GANSICKE B.T., MANSER C.J., CUNNINGHAM T., CUKANOVAITE E., HOLLANDS M., MARSH T., RADDI R., JORDAN S., TOONEN S., GEIER S., BARSTOW M., CUMMINGS J.D. Ref:=2021MNRAS.508.3877G byGENTILE FUSILLO N.P. , TREMBLAY P.-E., CUKANOVAITE E., VORONTSEVA A., LALLEMENT R., HOLLANDS M., GANSICKE B.T., BURDGE K.B., McCLEERY J., JORDAN S. Ref:=2020MNRAS.497..130T byTREMBLAY P.-E. , HOLLANDS M.A., GENTILE FUSILLO N.P., McCLEERY J., IZQUIERDO P., GANSICKE B.T., CUKANOVAITE E., KOESTER D., BROWN W.R., CHARPINET S., CUNNINGHAM T., FARIHI J., GIAMMICHELE N., VAN GROOTEL V., HERMES J.J., HOSKIN M.J., JORDAN S., KEPLER S.O., KLEINMAN S.J., MANSER C.J., MARSH T.R., DE MARTINO D., NITTA A., PARSONS S.G., PELISOLI I., RADDI R., REBASSA-MANSERGAS A., REN J.-J., SCHREIBER M.R., SILVOTTI R., TOLOZA O., TOONEN S., TORRES S. Ref:=2023MNRAS.518.3055O byO'BRIEN M.W. , TREMBLAY P.-E., GENTILE FUSILLO N.P., HOLLANDS M.A., GANSICKE B.T., KOESTER D., PELISOLI I., CUKANOVAITE E., CUNNINGHAM T., DOYLE A.E., ELMS A., FARIHI J., HERMES J.J., HOLBERG J., JORDAN S., KLEIN B.L., KLEINMAN S.J., MANSER C.J., DE MARTINO D., MARSH T.R., McCLEERY J., MELIS C., NITTA A., PARSONS S.G., RADDI R., REBASSA-MANSERGAS A., SCHREIBER M.R., SILVOTTI R., STEEGHS D., TOLOZA O., TOONEN S., TORRES S., WEINBERGER A.J., ZUCKERMAN B. Originof the Acronym: p = Pre-registered to IAU Comm.5
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 (Davis+Richer+Rich+, 2009) ***** Avoid the usage of WD, prefer [DRR2009] Originof the Acronym: A (2009ApJ...705..408K)
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: WhiteDwarf = 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., -1-None (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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