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Hasil Pencarian

 
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Friedman, John L., author
Summary: "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 during the coalescence of double neutron-star systems. This...
New York: Cambridge University Press, 2013
523.887 4 FRI r
Buku Teks  Universitas Indonesia Library