Details on Acronym: [WBB98] | |
| [WBB98] | (Weigelt+Balega+Blocker+, 1998)= (WHB) |
| Write: | <<[WBB98] A>> |
| N: | 7 |
| Object: | Knot (SIMBAD class: PartofCloud = Part of Cloud) |
| Stat: | is completely incorporated in Simbad |
| Note: | Study of the clumpy structure of IRC +10216: Component A is the central object, B, C, D, are bright knots, E, F are clouds. In 2000A&A...357..169O evolution of all the compact structures, and No. G added. |
| in source: | IRC +10216 |
| Ref: | =1998A&A...333L..51W |
| by | WEIGELT G. , BALEGA Y., BLOECKER T., FLEISCHER A.J., OSTERBART R., WINTERS J.M. |
| Astron. Astrophys., 333, 51-54 (1998) | |
| 76mas speckle-masking interferometry of IRC+10216 with the SAO 6m telescope: Evidence for a clumpy shell structure. | |
| o | Fig.1: <[WBB98] A> (Nos A-F). |
| Ref: | =2000A&A...357..169O |
| by | OSTERBART R. , BALEGA Y.Y., BLOECKER T., MEN'SHCHIKOV A.B., WEIGELT G. |
| Astron. Astrophys., 357, 169-176 (2000) | |
| The dynamical evolution of the fragmented, bipolar dust shell around the carbon star IRC +10 216. Rapid changes of a PPN-like structure? | |
| o | Fig.2, Table 2: <[WBB98] A> (No. G) added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: WHB | |
| WHB | (Weigelt+Haniff+Bushcher) |
| ***** | Avoid the usage of WHB, prefer [WBB98] |
| Origin | of the Acronym: L (2000ApJ...543..284T) |