Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon: I. V2028 Cyg
| Authors | |
|---|---|
| Year of publication | 2012 |
| Type | Article in Periodical |
| Magazine / Source | Astronomy and Astrophysics |
| MU Faculty or unit | |
| Citation | |
| Web | A&A |
| Doi | http://dx.doi.org/10.1051/0004-6361/201117210 |
| Field | Astronomy and astrophysics |
| Keywords | Line profiles binaries general circumstellar matter Stars emission-line B[e] Stars individual V2028 Cyg |
| Attached files | |
| Description | We present results of nearly six years of spectroscopic observations of the Be star V2028 Cyg. The presence of the cold-type absorption lines combined with a hot-type spectrum indicate the binarity of this object. Since B[e] stars are embedded in an extended envelope, the usage of common stellar atmosphere models for the analysis is quite inappropriate. Therefore, we focus on the analysis of the long-term spectral line variations in order to determine the nature of this object. |
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