Be stars in X-ray binary systems
| dc.creator | Coe, M. J. | |
| dc.date | 1999-11-15 | |
| dc.date.accessioned | 2026-07-07T02:34:27Z | |
| dc.date.available | 2026-07-07T02:34:27Z | |
| dc.description | This paper will review the status of our observations and understanding of Be stars in X-ray binary systems. In virtually all cases the binary partner to the Be star is a neutron star. The circumstellar disk provides the accretion fuel and hence stimulates the X-ray emission, whilst the neutron star provides a valuable probe of the environment around the Be star. The results coming from studies of such systems are helping in our understanding of the Be phenomenon. | |
| dc.description | Latex file, 10 figures, accepted for publication in Proceedings of IAU Colloq 175 "The Be phenomenon in early-type stars" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911272 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911272 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15246 | |
| dc.subject | Astrophysics | |
| dc.title | Be stars in X-ray binary systems | |
| dc.type | text |