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Details on Acronym: [VGM2003]
[VGM2003] (Verma+Ghosh+Mookerjea+, 2003) Write:<<[VGM2003] IRAS HHMMm+DDMM W>>
<<[VGM2003] ISO HHMMSS.s+DDMMSS>> N: 2+2+15 Object:Component (SIMBAD class: Infrared = Infra-Red Source) Stat:is completely incorporated in Simbad Note:TIFR balloon borne telescope and ISOCAM observations.
N=2 (FIR) peaks E and W in IRAS 19181+1349, and N=2 (IR) components N and S in IRAS 20286+4105.
N=10 ISOCAM sources in IRAS 19181+1349, N=2 in IRAS 20178+4016, and N=3 in IRAS 20286+4105. in source:IRAS 19181+1349 in source:IRAS 20286+4105 Ref:=2003A&A...398..589V byVERMA R.P. , GHOSH S.K., MOOKERJEA B., RENGARAJAN T.N. Astron. Astrophys., 398, 589-605 (2003) Far and mid infrared observations of two ultracompact HII regions and one compact CO clump. oTable 2: <[VGM2003] IRAS 19181+1349 W> (Nos E, W). Table 3: <[VGM2003] ISO HHMMSS.s+DDMMSSS> N=15. Table 4: <[VGM2003] IRAS 20286+4105 W> (Nos N, S). Originof the Acronym: S = Created by Simbad, the CDS Database
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