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Multiple-Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

M. Różyczka
M. Różyczka*
Affiliation:
Warsaw University ObservatoryAl. Ujazdowskie 4, PL-00-478 Warszawa, Poland

Abstract

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The present observational and theoretical status of multiple-supernova remnants is briefly reviewed, and evolutionary models of the remnants around OB associations are presented. The remnants are followed for up to almost 30 Myr in various galactic environments (Gaussian or composite disks combined with cold or hot halos). It is found that the presence of a hot halo profoundly modifies the evolution of the remnants, promoting the evaporation of their shells and leading to noneruptive merging of the ejecta with the halo gas. The results also suggest an explanation for the observed deficiency of evolved multiple-supernova remnants.

Type
VII. The Structure of the Interstellar Medium
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 463 - 473
Copyright
Copyright © Springer-Verlag 1989

References

Bertschinger, E. 1986, Astrophys. J. 304, 154 CrossRefGoogle Scholar
Bloemen, J.B.M.G. 1987, Astrophys. J. 322, 694 Google Scholar
Bruhweiler, F.C., Gull, T. Kafatos, M. and Sofia, S. 1980, Astrophys. J. Letters 238, L27 CrossRefGoogle Scholar
Cowie, L.L., Songaila, A., and York, D.G. 1979, Astrophys. J. 230, 469 Google Scholar
Fuchs, B., and Thielheim, K.O. 1979, Astrophys. J. 227, 801 Google Scholar
Heiles, C. 1984, Astrophys. J. Suppl. 55, 585 CrossRefGoogle Scholar
Heiles, C. 1987, Astrophys. J. 315, 555 Google Scholar
Igumentshchev, I.V., Shustov, B.M., and Tutukov, A.V.: 1989, Astron.Astrophys. (submitted)Google Scholar
Ikeuchi, S. 1987, in Starbursts and Galaxy Evolution, ed. Thuan, T.X., Montmerle, T., Tran Thanh Van, J., p.27, Gif sur Yvette: Ed. Front Google Scholar
Lockman, F.J., Hobbs, L.M., Shull, J.M. 1986, Astrophys. J301, 380 Google Scholar
McCray, R. and Kafatos, M. 1987, Astrophys. J. 317, 190 Google Scholar
Mac Low, M.-M. and McCray, R. 1988, Astrophys. J. 324, 776 Google Scholar
Mac Low, M.-M., McCray, R., and Norman, M.L. 1989, Astrophys. J. 337, 141 Google Scholar
Różyczka, M. 1985, Astron. Astrophys. 143, 59 Google Scholar
Tenorio-Tagle, G. and Bodenheimer, P. 1988, Ann. Rev. Astron. Astrophys. 26, 145 Google Scholar
Tenorio-Tagle, G., Bodenheimer, P., and Różyczka, M. 1987, Astron. Astrophys. 182, 120 Google Scholar
Tenorio-Tagle, G., Różyczka, M., and Bodenheimer, P. 1989, Astron. Astrophys., submittedGoogle Scholar
Tomisaka, K., Habe, H., and Ikeuchi, S. 1981, Astrophys. Sp. Sci. 78, 273 Google Scholar
Tomisaka, K., and Ikeuchi, S. 1986, Publ. Astr. Soc. Japan 38, 697 Google Scholar
Umemura, S., Kazuo, I., and Kazunari, S. 1988, Publ. Astr. Soc. Japan 40, 25 Google Scholar