Winds in OB-type stars
| dc.creator | Kaper, Lex | |
| dc.date | 1997-12-16 | |
| dc.date.accessioned | 2026-07-07T02:25:36Z | |
| dc.date.available | 2026-07-07T02:25:36Z | |
| dc.description | The International Ultraviolet Explorer satellite has made a tremendous contribution to the study of hot-star winds. Its long lifetime has resulted in the collection of ultraviolet spectra for a large sample of OB stars. Its unique monitoring capability has enabled detailed time-series analyses to investigate the stellar-wind variability for individual objects. IUE has also been a major driver for the development of the radiation-driven-wind theory; the synergy between theory and observations is one of the main reasons for the large progress that has been made in our understanding of hot-star winds and their impact on the atmospheres and evolution of massive stars. | |
| dc.description | 8 pages, latex, ps-figures and style files included; Invited Review "Ultraviolet astrophysics beyond the IUE final archive", Sevilla, November 1997 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9712201 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9712201 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11939 | |
| dc.subject | Astrophysics | |
| dc.title | Winds in OB-type stars | |
| dc.type | text |