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(ed.). Gravitational waves (IOP, 2001)(422s).

(ed.). Gravitational waves (IOP, 2001)(422s).

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References 83[19] van der Klis M 1998 The Many Faces of Neutron Stars <strong>ed</strong> R Buccheri, J van Paradijsand M A Alpar (Dordrecht: Kluwer Academic)[20] Bildsten L 1998 <strong>Gravitational</strong> radiation and rotation of accreting neutron starsAstrophys. J. 501 L89–93 (astro-ph/9804325)See also the recent paper Ushomirsky G, Cutler C and Bildsten L 1999 Deformationsof accreting neutron star crusts and gravitational wave emission Preprint (astroph/0001136)[21] Brady P R, Creighton T, Cutler C and Schutz B F 1998 Searching for periodic sourceswith LIGO Phys. Rev. D 57 2101–16[22] Brustein R, Gasperini M, Giovannini M and Veneziano G 1996 <strong>Gravitational</strong>radiation from string cosmology Proc. Int. Europhysics Conf. (HEP 95) <strong>ed</strong>CVander Velde, F Verbeure and J Lemonne (Singapore: World Scientific)[23] Schutz B F and Sorkin R 1977 Variational aspects of relativistic field theories, withapplication to perfect fluids Ann. Phys., NY 107 1–43[24] Isaacson R Phys. Rev. 166 1263–71Isaacson R 1968 Phys. Rev. 166 1272–80[25] Thorne K S 1980 Multipole expansions of gravitational radiation Rev. Mod. Phys. 52299–340[26] Schutz B F 1986 Determining the Hubble constant from gravitational waveobservations Nature 323 310–11[27] Chandrasekar S 1970 Phys. Rev. Lett. 24 611[28] Fri<strong>ed</strong>man J L and Schutz B F 1978 Ap. J. 222 281[29] Fri<strong>ed</strong>man J L and Morsink S M 1998 Axial instability of rotating relativistic starsAstrophys. J. 502 714–20 (gr-qc/9706073)[30] Andersson N, Kokkotas K and Schutz B F 1999 <strong>Gravitational</strong> radiation limit on thespin of young neutron stars Astrophys. J. 510 846–8539 (astro-ph/9805225)[31] Owen B, Lindblom L, Cutler C, Schutz B F, Vecchio A and Andersson N 1998<strong>Gravitational</strong> <strong>waves</strong> from hot young rapidly rotating neutron stars Phys. Rev. D5808 4020 (gr-qc/9804044)

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