Details on Acronym: [WBP2002] | |
| [WBP2002] | (Weigelt+Balega+Preibisch+, 2002) |
| Write: | <<[WBP2002] S 140 IRS N>> |
| N: | 4 |
| Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
| Note: | N=4 IR sources in Sh 2-140, considered for the authors as added to [BBW79] S 140 IRS 1 to 3, but in SIMBAD there are already different [BBW79] S 140 IRS 4 to 7, so the authors' IR sources are designated as [WBP2002] S 140 IRS N (Nos 4-7). |
| in source: | SH 2-140 |
| Ref: | =2002A&A...381..905W |
| by | WEIGELT G. , BALEGA Y.Y., PREIBISCH T., SCHERTL D., SMITH M.D. |
| Astron. Astrophys., 381, 905-913 (2002) | |
| Bispectrum speckle interferometry of the massive protostellar object S140 IRS1: Evidence for multiple outflows. | |
| o | IRS 1 to 3 = [BBW79] S 140 IRS 1 to 3, VLA NW = [BBW79] S 140 NW, VLA 4 = [BBW79] S 140 IRS 4 = [SFC83] S140 4, but IRS 4 to 7 here are different of [BBW79] S 140 IRS 4 to 7 in SIMBAD. |
| o | Fig.3: <[SBH2000] A> (Nos H-N) added. Fig.3: <[WBP2002] S 140 IRS N> (Nos 4-7). |