Percolating star formation in barred spirals

Details Percolating star formation in barred spirals Percolating star formation in barred spirals

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..441m&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 441-444 (1997).

Astronomy and Astrophysics

Astrophysics

1

Spiral Galaxies, Origin, Formation, Evolution, Age, And Star Formation, Star Formation

Scientific paper

The Stochastic Self-Propagating Star Formation (SSPSF) model [1], for self-regulating star formation based on a percolation process mitigated by supernova shocks, has been very successful in producing quantitative agreement with observations [2] when a Spiral Density Wave (SDW) has been a part of the imposed potential. It has been noted that many Spirals have a significant central bar. In this paper we extend the model to examine whether a barred potential alone is sufficient to produce long-lived spirals in the presence of propagating star formation.

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