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Supernovae Blast Waves in Proto-Dwarf Galaxies

Published online by Cambridge University Press:  12 April 2016

Alberto Noriego-Crespo  and
Peter Bodenheimer
Alberto Noriego-Crespo
Affiliation:
Canadian, Institute for Theoretical Astrophysics
Peter Bodenheimer
Affiliation:
Lick Observatory

Abstract

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Gas mass loss in proto-dwarf galaxies can be efficiently driven out by blast waves created by the first generation of supernovae. There is, however, a threshold set by the total gravitational potential beyond which gas mass loss does not occur. This limit is in agreement with the one predicted by some Cold Dark Matter senarios.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 513 - 520
Copyright
Copyright © Cambridge University Press 1988

References

Aaronson, M., 1986, in Stellar Populations, ed by Norman, C.A., Renzini, A., and Tosi, M.. Cambridge University Press.Google Scholar
Dekel, A., and Silk, J., 1986, Ap. J., 303, 39.CrossRefGoogle Scholar
King, I., 1966, Astron. J. 71, 64.CrossRefGoogle Scholar
Kormendy, J., 1987, in Nearly Normal Galaxies: From the Planck to the Present, ed. Faber., S.M. New York: Spring-Verlag, in press.Google Scholar
Noriega-Crespo, A., and Bodenheimer, P., 1987, in preparation.Google Scholar
Shields, G., Silk, J., Wyse, R.F.G., 1987, preprint.Google Scholar
Vader, J.P., 1986, Ap.J., 305, 669.CrossRefGoogle Scholar
Wyse, R.F.G., and Silk, J., 1985, Ap. J. Lett., 296, L1. (WS).CrossRefGoogle Scholar