Theory of dwarf galaxies

Details Theory of dwarf galaxies Theory of dwarf galaxies

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242..517g&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Dec. 1, 1980, p. 517-527.

Astronomy and Astrophysics

Astrophysics

226

Galactic Evolution, Galaxies, Star Distribution, Stellar Evolution, Astronomical Models, Brightness Temperature, Star Formation Rate

Scientific paper

Dwarf galaxies are characterized by properties which range from low surface brightness to the high surface brightness blue compact objects. The stochastic self-propagating star formation (SSPSF) model predicts that small systems can undergo a fluctuation which will completely stop propagation of star formation; the small galaxies will be restricted to star formation in a bursting mode of short-lived episodes during SSPSF. The bursting mode produces a star formation rate which varies with time leading to the diverse properties of dwarf galaxies.

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