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The optical counterpart of XTE J0929-314: the third transient millisecond X-ray pulsar
Authors:A. B. Giles  J. G. Greenhill  K. M. Hill   E. Sanders
Affiliation:School of Mathematics and Physics, University of Tasmania, GPO Box 252-21, Hobart, Tasmania 7001, Australia;Spurion Technology Pty. Ltd., 200 Mt. Rumney Road, Mt. Rumney, Tasmania 7170, Australia
Abstract:
Keywords:binaries close    pulsars general    pulsars individual XTE J0929-314    stars low-mass    stars neutron    X-rays binaries
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