Dictionary of Nomenclature of Celestial Objects
(Last update: 30-Jul-2021)

Result of query: info cati LLN92] IRS$



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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: IR = 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

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