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

Result of query: info cati WRAY$
 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>
 Auth.:GAUME R.A.+
   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.
 01.01.86 01.01.86
   Ref:=1990MNRAS.243..459M
     byMORGAN D.H.
, GOOD A.R.
 Mon. Not. R. Astron. Soc., 243, 459-461 (1990)

    Wolf-Rayet stars in the Large Magellanic Cloud.

o<MGWR N> No.8 added
   Ref:=1999MNRAS.305..469M
     byMORGAN D.H.

 Mon. Not. R. Astron. Soc., 305, 469-472 (1999)

    A new faint Wolf-Rayet star in the Large Magellanic Cloud.

o<MGWR N> (No. 9) added.

Details on Acronym:   WR
   WR (Wolf-Rayet *) Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Wr
   Wr (Wray) ***** Avoid the usage of Wr, prefer Wray
Details on Acronym:   WR33
   WR33 (WR* in M 33)

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