Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer [WBN72] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: WBN | |
WBN | (Wynn-Williams+Becklin+Neugebauer) |
***** | Avoid the usage of WBN, prefer [WBN72] |
Origin | of 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 |
by | WYNN-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 |
by | BEETZ 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 |
by | DYCK 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. | |
o | IRS in W 51 and W 75 = '[WBN74] W 51 IRS N' and [WBN74] W 75 IRS N' |
o | Table 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 |
by | HAYWARD 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. | |
o | Table 2: <[WBN72] W 3 IRS NNa> (Nos 2b-2c, 11). Table 2: <[HGW89] W 3 Star A> (Nos A-E). |
Ref: | =1994ApJ...424L..41C |
by | CLAUSSEN 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 |
o | Table 1: <[WBN72] W 3 IRS NaN> (Nos 5a-5c, 5d1-5d2, 5e-5f). |
Ref: | =1996A&A...307..775M |
by | MEGEATH 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 |
by | TIEFTRUNK 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. | |
o | Table 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. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |