AM CVn systems as optical, X-ray and GWR sources
| dc.creator | Yungelson, L. | |
| dc.creator | Nelemans, G. | |
| dc.creator | Zwart, S. F. Portegies | |
| dc.date | 2004-01-05 | |
| dc.date.accessioned | 2026-07-07T02:11:46Z | |
| dc.date.available | 2026-07-07T02:11:46Z | |
| dc.description | We discuss the model for the Galactic sample of the AM CVn systems with orbital periods P less than 1500 s, that can be detected in the optical and/or X-ray bands and may be resolved by the gravitational waves detector LISA. At P=3 to 10 min all detectable systems are X-ray sources. At P greater than 10 min most systems are only detectable in the V-band. About 30% of the X-ray sources is also detectable in the V-band. About 10,000 AM CVn systems might be resolved by LISA; this is comparable to the number of detached double white dwarfs that can be resolved. Several hundreds of AM CVn LISA sources might be also detectable in the V- and/or X-ray bands. | |
| dc.description | 3 pages, 2 figures, to appear in proceedings of the IAU Coll. 194 "Compact Binaries in the Galaxy and beyond", La Paz (Mexico), November 17-21, 2003 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0401027 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0401027 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7219 | |
| dc.subject | Astrophysics | |
| dc.title | AM CVn systems as optical, X-ray and GWR sources | |
| dc.type | text |