Spectral analysis of the LMC [WC] star SMP 61
- HST UV and optical spectra of the early-type [WC] star SMP 61 in the LMC are analyzed by means of line blanketed non-LTE models for expanding atmospheres. The known distance to the LMC allows a reliable determination of the stellar parameters. The low iron surface abundance of the object possibly indicates a preceding evolution through a very late thermal pulse (VLTP).
| Author details: | Götz Gräfener, Wolf-Rainer HamannORCiDGND |
|---|---|
| ISBN: | 1-583-81148-6 |
| Publication type: | Article |
| Language: | English |
| Year of first publication: | 2003 |
| Publication year: | 2003 |
| Release date: | 2017/03/24 |
| Source: | Planetary nebulae : their evolution and role in the universe ; proceedings of the 209th symposium of the International Astronomical Union held at Canberra, Australia, 19 - 23 November 2001 / Hrsg.: Michael Dopita ; Sun Kwok. - San Francisco : Astronomical Society of the pacific, 2003. - ISBN: 1-583-81148-6. - (ASP Conference Series ; 209) |
| Organizational units: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie |
| Peer review: | Nicht referiert |
| Institution name at the time of the publication: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik |
