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Observations of X-ray Burst Sources

Published online by Cambridge University Press:  04 August 2017

Y. Tanaka*
Affiliation:
Institute of Space and Astronautical Science, 4-6-1 Komaba, Meguro-ku, Tokyo 153, Japan

Abstract

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Recent observational results on X-ray bursts and burst sources are reviewed. Two distinct types of bursts, Type I and Type II bursts, are discussed in relation to the mass and radius of neutron stars and to the problems of unusual mass accretion in some burst sources.

Type
II. Accretion Powered Pulsars
Copyright
Copyright © Reidel 1987 

References

Dotani, T. et al. 1985, Proc. ISAS Conf. on Space Astrophys. (in Japanese).Google Scholar
Ebisuzaki, T. 1986, submitted to P.A.S.J. Google Scholar
Ebisuzaki, T., Hanawa, T. and Sugimoto, D. 1984, P.A.S.J., 36, 551.Google Scholar
Ebisuzaki, T. and Nomoto, K. 1986, Ap. J., in press.Google Scholar
Fujimoto, M.Y. 1985, Ap. J. (Letters), 293, L19.Google Scholar
Gottwald, M., Haberl, F., Parmer, A.N. and White, N.E. 1986, Ap. J., in press.Google Scholar
Grindlay, J., Marshall, H., Hertz, P. et al. 1980, Ap. J. (Letters), 240, L121.Google Scholar
Hoffman, J.A., Marshall, H.L. and Lewin, W.H.G. 1978, Nature, 271, 630.Google Scholar
Ikegami, T. 1986, private communication.Google Scholar
Inoue, H. et al. 1986, in preparation.Google Scholar
Inoue, H., Koyama, K., Makino, F. et al. 1984a, P.A.S.J., 36, 855.Google Scholar
Inoue, H., Koyama, K., Makishima, K. et al. 1981, Ap. J. (Letters), 250, L71.CrossRefGoogle Scholar
Inoue, H., Waki, I., Koyama, K. et al. 1984b, P.A.S.J., 36, 831.Google Scholar
Kawai, N. 1985, , Univ. of Tokyo (ISAS RN. No.302).Google Scholar
Kunieda, H., Tawara, Y., Hayakawa, S. et al. 1984, P.A.S.J., 36, 807.Google Scholar
Lewin, W.H.G., Doty, J., Clark, G.W. et al. 1976a, Ap. J. (Letters), 207, L95.Google Scholar
Lewin, W.H.G., Hoffman, J.A., Doty, J. et al. 1976b, M.N.R.A.S., 179, 83.Google Scholar
Lewin, W.H.G. and Joss, P.C. 1983, “Accretion-Driven Stellar X-Ray Sources”, ed. Lewin, and van den Heuvel, (Cambridge Univ. Press), p.41.Google Scholar
Lewin, W.H.G., Vacca, W.D. and Basinska, E.M. 1984, Ap. J. (Letters), 277, L57.Google Scholar
London, R.A., Taam, R.E. and Howard, W.M. 1984, Ap. J. (Letters), 287, L27.Google Scholar
Murakami, T., Inoue, H., Koyama, K. et al. 1980, P.A.S.J., 32, 543.Google Scholar
Nakamura, N. et al. 1986, in preparation.Google Scholar
Ohashi, T., Inoue, H., Koyama, K. et al. 1982, Ap. J., 258, 254.Google Scholar
Stella, L., Parmer, A.N., White, N.E. et al. 1985, IAU Circular No.4110.Google Scholar
Sugimoto, D., Ebisuzaki, T. and Hanawa, T. 1984, P.A.S.J., 36, 839.Google Scholar
Tanaka, Y. 1985, Twelfth Texas Symposium on Relativistic Astrophys., p163.Google Scholar
Tawara, Y. et al. 1986, in preparation.Google Scholar
Tawara, Y., Hayakawa, S., Kunieda, H. et al. 1982, Nature, 299, 38.Google Scholar
Tawara, Y., Kawai, N., Tanaka, Y. et al. 1985, Nature, 318, 545.Google Scholar
Tawara, Y., Kii, T., Hayakawa, S. et al. 1984, Ap. J. (Letters), 276, L41.Google Scholar
Tennant, A.F., Fabian, A.C. and Shafer, P.A. 1986a, M.N.R.A.S., 219, 871.Google Scholar
Tennant, A.F., Fabian, A.C. and Shafer, P.A. 1986b, to appear in M.N.R.A.S. Google Scholar
Vacca, W.D., Lewin, W.H.G. and van Paradijs, J. 1985, to appear in M.N.R.A.S. Google Scholar
van Paradijs, J. 1978, Nature, 274, 650.Google Scholar
van Paradijs, J. and Lewin, W.H.G. 1986, A.& Ap., 157, L10.Google Scholar
Waki, I., Inoue, H., Koyama, K. et al. 1984, P.A.S.J., 36, 819.Google Scholar