Published 1988 | Version v1
Book Metadata-only

Supernovae blast waves in proto-dwarf galaxies

Creators

  • 1. Canadian Institute for Theoretical Astrophysics (Canada)
  • 2. California Univ., Santa Cruz, CA (USA). Lick Observatory

Description

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 paper discusses how this limit is in agreement with the one predicted by some cold dark matter scenarios

Additional details

Publishing Information

Publisher
Cambridge University Press.
Imprint Place
New York, NY (USA)
ISBN
0-521-35062-X
Imprint Title
Supernova remnants and the interstellar medium
Imprint Pagination
535 p.
Journal Page Range
p. 517-520.

Conference

Title
101. International Astronomics Union colloquium on interaction of supernova remnants with the interstellar medium.
Dates
8-12 Jun 1987.
Place
Penticton (Canada).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22001244
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
GALACTIC EVOLUTION; MASS; NONLUMINOUS MATTER; PROTOSTARS; SHOCK WAVES; STAR EVOLUTION; SUPERNOVAE
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; MATTER; STARS; VARIABLE STARS

Optional Information

Secondary number(s)
CONF-8706201--.