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 |
| by | VERMA 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. | |
| o | Table 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). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |