Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer [LLN92] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: LLN | |
LLN | (Liseau+Lorenzetti+Nisini+) |
Origin | of the Acronym: L (2006A&A...449..251T) |
Details on Acronym: [LLN92] | |
[LLN92] | (Liseau+Lorenzetti+Nisini+, 1992)= (IRS) = (LLN) |
Write: | <<[LLN92] IRS NN>> <<[LLN92] IRS NN-N>> |
N: | 122 |
Object: | (Near IR) (SIMBAD class: Infrared = Infra-Red Source) |
Note: | N=122 (NIR) sources in 92 IRAS fields in the Vela Molecular Ridge (VMR). When there is only one (NIR) in the IRAS field, the format is 'NN' (among (Nos 1-92)). When there are several (NIR) in the IRAS field, the format is 'NN-N'. Identif. charts. See also VMR, [MGL99], [LGV2002], [MLG2003]. |
in source: | NAME VMR |
Ref: | =1992A&A...265..577L |
by | LISEAU R. , LORENZETTI D., NISINI B., SPINOGLIO L., MONETI A. |
Astron. Astrophys., 265, 577-596 (1992) | |
Star formation in the Vela molecular clouds. I. The IRAS-bright class I sources. | |
o | IRAS 08485-4359 misprint for 08485-4419 |
o | Table 1: <[LLN92] IRS NN> (Nos 1-55), <[LLN92] IRS NN-N> N=22. |
Ref: | =1993A&A...275..489L |
by | LORENZETTI D. , SPINOGLIO L., LISEAU R. |
Astron. Astrophys., 275, 489-509 (1993) | |
Star formation in the Vela molecular clouds. II. The luminosity function of the class I sources. | |
o | Table 1: <[LLN92] IRS NN> (Nos 56-92), <[LLN92] IRS NN-N> N=40. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |