X - Ray and Gwr Sources
نویسندگان
چکیده
3 RESUMEN ABSTRACT We discuss the model for the Galactic sample of the AM CVn systems with P orb ≤ 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 3 ∼ < P ∼ < 10 min all detectable systems are X-ray sources. At P ∼ > 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.
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