Rotating relativistic stars
"The masses of neutron stars are limited by an instability to gravitational collapse, and an instability driven by gravitational waves limits their spin. Their oscillations are relevant to X-ray observations of accreting binaries and to gravitational wave observations of neutron stars formed du...
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| Format: | Electronic eBook |
| Language: | English |
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Cambridge :
Cambridge University Press,
2013.
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| Series: | Cambridge monographs on mathematical physics
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| Online Access: | Click to View |
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