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Supernova and Cosmic Rays

Published online by Cambridge University Press:  14 August 2015

John P. Wefel
John P. Wefel*
Affiliation:
Enrico Fermi Institute, University of Chicago, Chicago, Illinois, 60637 USA

Extract

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The Supernova (SN) is one of the most important and most complex phenomena in astrophysics. Detailed observations of SN require advanced techniques of astronomy and high energy astrophysics, but the theoretical explanation of SN involves virtually every branch of physics. Supernovae, however, offer more than a challenging physics problem because SN are involved in the origin of most of the heavy elements, are the birthplaces of neutron stars, pulsars and probably black holes, control the structure of the interstellar medium, may be responsible for the birth of new stars (and possibly our own solar system), and, of greatest concern in this paper, are involved either directly or indirectly in the origin of the galactic cosmic rays.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 94: Origin of Cosmic Rays , 1981, pp. 39 - 50
Copyright
Copyright © Reidel 1981 

References

Arnett, W.D.: 1977, Ap. J. Suppl., 35, pp. 145–159.Google Scholar
Arnett, W.D.: 1978, Ap. J., 219, pp. 1008–1016.Google Scholar
Arnett, W.D.: 1979, Ap. J. Lett., 230, pp. L37–L40.Google Scholar
Arnett, W.D., and Wefel, J.P.: 1978, Ap. J. Lett., 224, pp. L139–L142.Google Scholar
Barbon, R., Ciatti, F., and Rosino, L.: 1974, “Supernovae and Supernova Remnants”, ed. Cosmovici, C.B. (Dordrecht: Reidel), pp. 99–118.Google Scholar
Blandford, R.D., and Ostriker, J.P.: 1978, Ap. J. Lett., 221, pp.L29–L32.Google Scholar
Casse, M., and Goret, P.: 1978, Ap. J., 221, pp. 703–712.CrossRefGoogle Scholar
Chevalier, R.A.: 1977, Ann. Rev. Astron. Astrophys., 15, pp. 175–196.Google Scholar
Dwek, E., and Scalo, J.M.: 1980, Ap. J., in press Google Scholar
Falk, S.W., and Arnett, W.D.: 1977, Ap. J. Suppl., 33, pp. 515–562.Google Scholar
Freedman, D.Z., Schramm, D.N., and Tubbs, D.L.: 1977, Ann. Rev. Nucl. Sci., 27, pp. 167–207.Google Scholar
Garcia-Munoz, M., Mason, G.M., and Simpson, J.A.: 1977, Ap. J., 217, pp. 859–877.Google Scholar
Ginzburg, V.L., and Syrovatskii, S.I.: 1964, “The Origin of Cosmic Rays” (New York: Macmillan), pp. 194–200.Google Scholar
Hainebach, K.L. Norman, E.B., and Schramm, D.N.: 1976, Ap. J., 203, pp. 245–256.Google Scholar
McKee, C.F., and Ostriker, J.P.: 1977, Ap. J., 218, pp. 148–169.Google Scholar
Norman, E.B., and Schramm, D.N.: 1979, Ap. J., 228, pp. 881–892.Google Scholar
Schramm, D.N.: 1978, “Protostars & Planets”, ed. Gehrels, T. (Tuscon: Univ. of Arizona Press), pp. 384–398.Google Scholar
Schramm, D.N., and Arnett, W.D.: 1974, “Explosive Nucleosynthesis”, eds. Schramm, D.N. and Arnett, W.D. (Austin: Univ. of Texas Press), pp. 45–229.Google Scholar
Schwartz, S.J., and Skilling, J.: 1978, Astron. Astrophys., 70, pp. 607–616.Google Scholar
Scott, J.S., and Chevalier, R.A.: 1975, Ap. J. Lett., 197, pp. L5–L8.Google Scholar
Thielemann, F.K., Arnould, M., and Hillebrandt, W.: 1979, Astron. Astrophys., 74, pp. 175–185.Google Scholar
Truran, J.W., and Iben, I.: 1977, Ap. J., 216, pp. 797–810.Google Scholar
Van Riper, K.A.: 1978, Ap. J., 221, pp. 304–319.Google Scholar
Weaver, T.A., Zimmerman, G.B., and Woosley, S.E.: 1978, Ap. J., 225, pp. 1021–1029.Google Scholar
Weaver, T.A., and Woosley, S.E.: 1979, Proc. 9th Texas Symp. on Rel. Astrophys., in press.Google Scholar
Wefel, J.P., Schramm, D.N., and Blake, J.B.: 1977, Astrophys. Sp. Sci, 49, pp. 47–81.Google Scholar
Wefel, J.P., Schramm, D.N., Blake, J.B., and Pridmore-Brown, D.: 1980, Ap. J., in press Google Scholar
Woosley, S.E., and Howard, W.M.: 1978, Ap. J. Suppl., 36, pp. 285–304.Google Scholar