On Star Formation in Nonlinear Systems / Gas Stars

Details On Star Formation in Nonlinear Systems / Gas Stars On Star Formation in Nonlinear Systems / Gas Stars

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1531....3p&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1531/SEPT, P.3 , 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

An analytical two-component model of star formation (SF) process with damping effects is presented. It is shown that the one-zone model producing a regime of rare bursts may be extended to a distributed model. Quantitative estimates of the SF wave velocity (2 - 3 km/s) and the size (≡200 pc) of the domain, where a stationary SF wave exists, are obtained.

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