X-ray line profiles from structured stellar winds
- Absorbing material compressed in a number of thin shells is effectively less opaque for X-rays than smoothly distributed gas. The calculated X-ray emission line profiles are red-shifted if the emission arises from the starward side of the shells.
Author details: | Lidia M. OskinovaORCiDGND, Achim FeldmeierORCiDGND, Wolf-Rainer HamannORCiDGND |
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ISBN: | 1-58381-133-8 |
Publication type: | Article |
Language: | English |
Year of first publication: | 2003 |
Publication year: | 2003 |
Release date: | 2017/03/24 |
Source: | A massive star odyssey : from main sequence to supernova ; proceedings of the International Astronomical Union held in Costa Tequise / Hrsg.: Karl A. van der Hucht; Artemio Herrero; Cesar Esteban. - San Francisco : Astronomical Society of the Pacific, 2003. - ISBN: 1-58381-133-8. - S. 214 |
Organizational units: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie |
Institution name at the time of the publication: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik |