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Evolution of Neutron Stars in Young Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

K. Nomoto  and
S. Tsuruta
K. Nomoto
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, West Germany
S. Tsuruta
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, West Germany

Extract

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The exciting observational developments in recent years (see Seward, Helfand, Harnden, Becker, etc., in this volume) have made it worthwhile to reexamine neutron star cooling theories. Here we shall give an intermediate report on our work.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 509 - 512
Copyright
Copyright © Reidel 1983 

References

Baym, G., Pethick, C.J., and Sutherland, P.G.: 1971. Ap. J. 170, p. 299.Google Scholar
Flowers, E.G., and Itoh, N.: 1976. Ap. J. 206, p. 218.Google Scholar
Huebner, W.F., et. al.: 1977. Astrophysical Opacity Library (Rep. No. LA 6760M, Los Alamos Scientific Laboratory).Google Scholar
Ichimaru, S., Itoh, N., Iyetomi, H., and Mitake, S.: 1982. in preparation.Google Scholar
Nomoto, K., and Tsuruta, S.: 1981. Ap. J. Letters 250, p. L19.Google Scholar
Nomoto, K., and Tsuruta, S.: 1982. in preparation.Google Scholar
Pandharipande, V.R., and Smith, R.A.: 1975. Nucl. Phys. A237, p. 507.Google Scholar
Takatsuka, T.: 1981. Proceedings of the 2nd International Conference on “Recent Progress in Many Body Theories”, Oaxtepec, Morelos, Mexico.Google Scholar
Tamagaki, R.: 1981. Proceedings of the 2nd International Conference on “Recent Progress in Many Body Theories”, Oaxtepec, Morelos, Mexico.Google Scholar
Thorne, K.S.: 1977. Ap. J. 212, p. 825.Google Scholar
Tsuruta, S.: 1980. X-Ray Astronomy (ed. Giacconi, R. and Setti, G., Dordrecht: Reidel), p. 73.Google Scholar
Tsuruta, S.: 1981. Pulsars (ed. Sieber, W. and Wielebinski, R., Dordrecht: Reidel), p. 331.Google Scholar
Yakovlev, D.G., and Urpin, V.A.: 1980. Sov. Astron. 24, p. 303.Google Scholar