Observing Globular Cluster Binaries with Gravitational Radiation

作者: Matthew Benacquista

DOI: 10.1007/978-94-015-9723-4_5

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摘要: Ultracompact binaries are expected to be the best candidates for continuous gravitational radiation in frequency range of space-based gravity wave detectors such as LISA. The dynamics globular cluster evolution enhance population clusters. We present nature which will detectable by LISA well fraction galactic system can explored

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