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Accretion onto Magnetized Neutron Stars

Published online by Cambridge University Press:  25 April 2016

J. G. Kirk
J. G. Kirk*
Affiliation:
Department of Theorectical Physics, University of Sydney, Sydney N.S.W. 2006, Australia
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Extract

Magnetic fields of about 1012 G have now been measured in several astrophysical objects (Trümper etal. 1978, Wheaton et al. 1979, Mazets et al. 1981). In the case of pulsating X-ray sources, the presence of a companion star indicates that accretion is probably the energy source for the X-rays.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 446 - 456
Copyright
Copyright © Astronomical Society of Australia 1984

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References

Abramowitz, M., and Stegun, I. A., 1972, ‘Handbook of Mathematical Functions’, Dover, New York.Google Scholar
Alme, M. L., and Wilson, J. R., 1973, Astrophys. J., 186, 1015.Google Scholar
Anzer, U., and Börner, G., 1983, Astron. Astrophys., 122, 73.Google Scholar
Arons, J., and Lea, S. M., 1980, Astrophys. J., 235, 1016.CrossRefGoogle Scholar
Basko, M. M., and Sunyaev, R. A., 1975, Astron. Astrophys., 42, 311.Google Scholar
Basko, M. M., and Sunyaev, R. A., 1975b, Sov. Phys. JETP. 41, 52.Google Scholar
Basko, M. M., and Sunyaev, R. A., 1976, Mon. Not. R. Astron. Soc., 175, 395.Google Scholar
Braun, A., and Yahel, R. Z., 1984, Astrophys. J., 278, 349.Google Scholar
Castor, J. I., 1972, Astrophys. J., 178, 779.Google Scholar
Davidson, K., 1973, Nature Phys. Sci., 246, 1.Google Scholar
Fryxell, B. A., and Woosley, S. E., 1982, Astrophys. J., 258, 733.CrossRefGoogle Scholar
Harding, A. K., Mészáros, P., Kirk, J. G., and Galloway, D. J., 1984, Astrophys. J., 278, 369.Google Scholar
Inoue, H., 1975, Publ. Astron. Soc. Japan. 27, 311.Google Scholar
Kirk, J. G., 1984, submitted to Astron. Astrophys.Google Scholar
Kirk, J. G., and Galloway, D. J., 1982, Plasma Phys., 24, 339 and 1025.Google Scholar
Kirk, J. G., Melrose, D. B., and Peters, J., 1984, Proc. Astron. Soc. Aust., 5, 000.Google Scholar
Lamb, F. K., Pethick, C. J., and Pines, D., 1973, Astrophys. J., 184, 271.Google Scholar
Langer, S. H., and Rappaport, S., 1982, Astrophys. J., 257, 733.Google Scholar
Mazets, E. P., Golenetskii, S. V., Aptekar, R. L., Gur’yan, Y. A., and Il’inskii, V. N., 1981, Nature, 290, 378.CrossRefGoogle Scholar
Meszaros, P., Harding, A. K., Kirk, J. G., and Galloway, D. J., 1983, Astrophys. J., 266, L33.Google Scholar
Pavlov, G. G., and Yakovlev, D. G., 1976, Sov. Phys. JETP. 43, 389.Google Scholar
Pomraning, G. C., 1973, ‘The Equations of Radiation Hydrodynamics’ Pergamon, Oxford.Google Scholar
Riffert, H., 1983, Ph.D. thesis Ludwig Maximilian Universität München. Google Scholar
Riffert, H., 1984, preprint Max-Planck-Institut für Astrophysik, Garching. Trümper, J., Pietsch, W., Reppin, C., Voges, W., Staubert, R., and Kendziorra, E., 1978, Astrophys. J., 219, 105.Google Scholar
Wang, Y. M., and Frank, J., 1981, Astron. Astrophys., 93, 225.Google Scholar
Wheaton, W. A., et al. 1979, Nature, 28, 240.Google Scholar
White, N. E., Swank, J. H., and Holt, S. S., 1983, Astrophys. J., 270, 711.Google Scholar
Zeldovich, Y. B., and Raizer, Y. P., 1967, ‘Physics of Shock Waves and High Temperature Phenomena’ Academic Press, New York.Google Scholar