Publication details
Mass Loss from Massive Zero-Metallicity Stars
| Authors | |
|---|---|
| Year of publication | 2006 |
| Type | Article in Proceedings |
| Conference | Stellar Evolution at Low Metallicity: Mass Loss, Explosions |
| MU Faculty or unit | |
| Citation | |
| Web | http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ASPC..353..133K&db_key=AST&data_type=HTML&format=&high=403a2464f518671 |
| Field | Astronomy and astrophysics |
| Keywords | stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter |
| Description | We show that the radiative force is not able to drive a stellar wind from non-rotating hot massive zero-metallicity stars. This means that stellar winds from stationary massive hot first generation stars are unlikely. We study the possibility of expulsion of chemically homogeneous winds and the role of minor isotopes. |
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