Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati WBN72] W 3 IRS NN$
.
.
.
.

Details on Acronym:   IRS
  
IRS (IR Source)
***** Avoid the usage of IRS, prefer [WBN72]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   WBN
  
WBN (Wynn-Williams+Becklin+Neugebauer)
***** Avoid the usage of WBN, prefer [WBN72]
Originof the Acronym: L = Found in the literature

Details on Acronym:   [WBN72]
  
[WBN72] (Wynn-Williams+Becklin+Neugebauer, 1972)= (IRS) = (WBN)
Write:<<[WBN72] W 3 IRS NNaN>>
N: 11+12
Object:(IR)  (SIMBAD class: Infrared = Infra-Red Source)
Stat:is completely incorporated in Simbad
in source:W 3
Ref:=1972MNRAS.160....1W
byWYNN-WILLIAMS C.G. , BECKLIN E.E., NEUGEBAUER G.
 Mon. Not. R. Astron. Soc., 160, 1-14 (1972)
  Infra-red sources in the H II region W 3.
o<[WBN72] W 3 IRS N> (Nos 1-9)
Ref:=1974A&A....34..335B
byBEETZ M. , ELSAESSER H., WEINBERGER R.
 Astron. Astrophys., 34, 335-337 (1974)
  The H II region W 3 in the near infrared.
o<[WBN72] W 3 IRS Na> (No. 2a) added.
Ref:=1977ApJ...211..421D
byDYCK H.M. , SIMON T.
 Astrophys. J., 211, 421-428 (1977)
  Infrared observations of compact H II regions in the spectral range 3.4-33 micrometers.
oIRS in W 51 and W 75 = '[WBN74] W 51 IRS N' and [WBN74] W 75 IRS N'
oTable 1: <[WBN72] W 3 IRS NN> (No. 10) added. Table 1: <[DS77] W 33 IRS N> (Nos 1-3). Table 2: <NAME DR 21 IRS>, <NAME DR 21 (N and S)>, <NAME W 75 (N)>.
Ref:=1989ApJ...345..894H
byHAYWARD T.L. , GRASDALEN G.L., WOODWARD C.E., HACKWELL J.A., GEHRZ R.D., PIPHER J.L.
 Astrophys. J., 345, 894-905 (1989)
  Infrared imaging of the compact HII region W3A.
oTable 2: <[WBN72] W 3 IRS NNa> (Nos 2b-2c, 11). Table 2: <[HGW89] W 3 Star A> (Nos A-E).
Ref:=1994ApJ...424L..41C
byCLAUSSEN M.J. , GAUME R.A., JOHNSTON K.J., WILSON T.L.
 Astrophys. J., 424, 41-44 (1994)
  The W3 IRS 5 cluster : radio continuum and water maser observations.
o'[WBN72] W 3 IRS 5g' is added in 1997A&A.318.931T
oTable 1: <[WBN72] W 3 IRS NaN> (Nos 5a-5c, 5d1-5d2, 5e-5f).
Ref:=1996A&A...307..775M
byMEGEATH S.T. , HERTER T., BEICHMAN C., GAUTIER N., HESTER J.J., RAYNER J., SHUPE D.
 Astron. Astrophys., 307, 775-790 (1996)
  A dense stellar cluster surrounding W3 IRS 5.
o<[WBN72] W 3 IRS Na> (Nos 3a-3b).
Ref:=1997A&A...318..931T
byTIEFTRUNK A.R. , GAUME R.A., CLAUSSEN M.J., WILSON T.L., JOHNSTON K.J.
 Astron. Astrophys., 318, 931-946 (1997)
  The H II/molecular cloud complex W3 revisited: imaging the radio continuum sources using multi-configuration, multi-frequency observations with the VLA.
oTable 3: <[TGC97] W3AaN> (Nos 3Ma-3Mc, 3Md1-3Md2, 3Me-3Mg, 3Ca) = <[WBN72] W 3 IRS NaN> (Nos 5a-5c, 5d1-5d2, 5e-5g, 4a) among which (Nos 5g, 4a) added.
Originof the Acronym: S = Created by Simbad, the CDS Database