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

Result of query: info cati LLN92]$

Details on Acronym:   IRS
  
IRS (IR Source)
***** Avoid the usage of IRS, prefer [LLN92]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   LLN
  
LLN (Liseau+Lorenzetti+Nisini+)
Originof 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
byLISEAU 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.
oIRAS 08485-4359 misprint for 08485-4419
oTable 1: <[LLN92] IRS NN> (Nos 1-55), <[LLN92] IRS NN-N> N=22.
Ref:=1993A&A...275..489L
byLORENZETTI 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.
oTable 1: <[LLN92] IRS NN> (Nos 56-92), <[LLN92] IRS NN-N> N=40.
Originof the Acronym: S = Created by Simbad, the CDS Database