Some evolutionary consequences of shock-induced star formation

Details Some evolutionary consequences of shock-induced star formation Some evolutionary consequences of shock-induced star formation

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138..201n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, p. 201-204.

Astronomy and Astrophysics

Astrophysics

3

Shock Waves, Star Formation, Asymptotes, Distribution Functions, Mass Distribution, Stellar Models

Scientific paper

In this paper evolutionary consequences of shock induced star formation are calculated for galaxy gas contents on the basis of simple two-component model. It is shown that a state where the mass density in stars is stationary is reached within less than 10 to the 9.5th yr and that the majority of systems evolve into a particular state. It is also shown how this asymptotic state is reached.

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