On a Modification to the Stochastic Self Propagating Star Formation Model

Details On a Modification to the Stochastic Self Propagating Star Formation Model On a Modification to the Stochastic Self Propagating Star Formation Model

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.235..161a&link_type=abstract

Astrophysics and Space Science, Volume 235, Issue 1, pp.161-163

Astronomy and Astrophysics

Astrophysics

Scientific paper

The stochastic self propagating star formation (SSPSF) model is modified
by assuming that a star is formed if a neighbouring star explodes. This
is a more reasonable assumption than the original model. The basic
features of SSPSF are shown to be preserved hence one still can explain
the galactic spiral arms and luminosity.

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