Details on Acronym: [BCB89] | |
[BCB89] | (Barnes+Crutcher+Bieging+, 1989)= BCBSW = (IRS) |
Write: | <<[BCB89] IRS NNa>> |
N: | 31+1 |
Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
Stat: | is completely incorporated in Simbad |
Note: | IRS 1 and IRS 2 where already existing, respectively discovered in 1968PASP...80...20G and 1974ApJ...193..373G, and also designated in SIMBAD as NGC 2024 1 and 2. IRS 2b is discovered later as the candidate ionizing star of NGC 2024. |
in source: | NGC 2024 |
Ref: | =1989ApJ...342..883B |
by | BARNES P.J. , CRUTCHER R.M., BIEGING J.H., STOREY J.W.V., WILLNER S.P. |
Astrophys. J., 342, 883-907 (1989) | |
Orion B (NGC 2024). I. VLA and IR observations of the HII region. | |
o | Table 1: <[BCB89] IRS NN> (Nos 1-31) |
Ref: | =2003A&A...404..249B |
by | BIK A. , LENORZER A., KAPER L., COMERON F., WATERS L.B.F.M., DE KOTER A., HANSON M.M. |
Astron. Astrophys., 404, 249-254 (2003) | |
Identification of the ionizing source of NGC 2024. | |
o | Fig. 1 : IRS N = [BCB89] IRS N. G206.543-16.347 = [KCW94] 206.543-16.347 |
o | <[BCB89] IRS NNa> (No. 2b) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: BCBSW | |
BCBSW | (Barnes+Crutcher+Bieging+Storey+Willner) |
====> | Equivalent to: [BCB89] |
Origin | of the Acronym: L (1995A&A...296L..21F) |
Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer [BCB89] |
Origin | of the Acronym: A = Assigned by the author(s) |