Details on Acronym: [SBH2000] | |
| [SBH2000] | (Schertl+Balega+Hannemann+, 2000) |
| Write: | <<[SBH2000] A>> |
| N: | 14 |
| Object: | Clump (SIMBAD class: PartofCloud = Part of Cloud) |
| Note: | N=14 clumps in SH 2-140 IRS 1 = [BBW79] S 140 IRS 1. |
| in source: | Sh 2-140:[BBW79] S 140 IRS 1 = [BBW79] S 140 IRS 1 |
| Ref: | =2000A&A...361L..29S |
| by | SCHERTL D. , BALEGA Y., HANNEMANN T., HOFMANN K.-H., PREIBISCH T., WEIGELT G. |
| Astron. Astrophys., 361, 29-32 (2000) | |
| Diffraction-limited bispectrum speckle interferometry and speckle polarimetry of the young bipolar outflow source S140 IRS1. | |
| o | Fig.1: <[SBH2000] A> (Nos A-G). |
| 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). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |