.
Details on Acronym: [BGE2002]
[BGE2002] (Beltran+Girart+Estalella+, 2002)= (BIMA) = (VLA) Write:<<[BGE2002] VLA N>>
<<[BGE2002] BIMA NW>>
<<[BGE2002] Clump A>> N: 5+3+1+2 Object:(Rad) + (mm) + Clump (SIMBAD class: Unknown = Object of Unknown Nature) Stat:is completely incorporated in Simbad Note:Centimeter observations of gas and dust around IRAS 21391+5802 embedded in the core of IC 1396N.
N=5 VLA sources.
N=3 BIMA (Berkeley-Illinois-Maryland Assoc.) mm sources (Nos 1-3), and a yet undetected YSO 'BIMA 1W'.
N=2 CS emission clumps, B (blueshifted) and R (Redshifted). in source:IC 1396N Ref:=2002ApJ...573..246B byBELTRAN M.T. , GIRART J.M., ESTALELLA R., HO P.T.P., PALAU A. Astrophys. J., 573, 246-259 (2002) IRAS 21391+5802: the molecular outflow and its exciting source. op. 247 : Calibrator 2148+611 not identified oTable 2: <[BGE2002] VLA N> (Nos 1-5). Table 3: <[BGE2002] BIMA N> (Nos 1-3). Fig.6: <[BGE2002] Clump A> (Nos B, R). Ref:=2004A&A...426..941B byBELTRAN M.T. , GIRART J.M., ESTALELLA R., HO P.T.P. Astron. Astrophys., 426, 941-949 (2004) The dense molecular cores in the IRAS 21391+5802 region. oText: <[BGE2002] BIMA 1W> added. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BIMA
BIMA (Berkeley-Illinois-Maryland Assoc.) ***** Avoid the usage of BIMA, prefer [BGE2002] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: VLA
VLA (Very Large Array) ***** Avoid the usage of VLA, prefer [BGE2002] Originof the Acronym: A = Assigned by the author(s)
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