Gravitational Radiation from Helium Cataclysmics

摘要: For a gravitational wave antenna in space, radiation from very large numbers of galactic binaries will be present the observable frequency band roughly 10-5 Hz to 1 Hz. At frequencies above about 3 mHz, signals thousands compact resolvable both and direction. lower frequencies, there confusion noise having more than one binary per resolution bin, even with year or data. In this paper, we extend previous discussions include an improved estimate contributions AM CVn their probable progenitors, which refer as helium cataclysmics. We find only slight increase below essentially no at higher frequencies.