X-ray Emission from Isolated Be Stars
| dc.creator | Cohen, David H. | |
| dc.date | 2000-08-22 | |
| dc.date.accessioned | 2026-07-07T01:55:02Z | |
| dc.date.available | 2026-07-07T01:55:02Z | |
| dc.description | I discuss the X-ray observations of Be stars, and how their properties compare to non-emission B stars. I focus on several specific stars that show high flux levels and variability but also report on several interesting survey results. The Be X-ray properties are discussed in the context of wind-shock X-ray emission from normal OB stars as well as in the context of general mechanisms that have been proposed to explain the Be phenomenon. Finally, I conclude with a discussion of the spectral diagnostics that will be available from the new generation of X-ray telescopes. | |
| dc.description | To appear in A.S.P. conf. ser. 214, The Be Phenomenon in Early-Type Stars, eds. Smith, Henrichs, Fabregat; Also available at http://hven.swarthmore.edu/~cohen/Papers/alicante.ps | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0008346 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0008346 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1521 | |
| dc.subject | Astrophysics | |
| dc.title | X-ray Emission from Isolated Be Stars | |
| dc.type | text |