Blue compact dwarf evolution in a UV background field

Details Blue compact dwarf evolution in a UV background field Blue compact dwarf evolution in a UV background field

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998egdg.conf..229h&link_type=abstract

"Dynamics of Galaxies and Galactic Nuclei, An International Workshop of the SFB 328 "Evolution of Galaxies" held at the ITA Nove

Physics

Scientific paper

A scenario for the formation of BCDs is presented in which an external
UV background field interrupts the ongoing star formation. Though the
preliminary model presented here fails to produce enough cold gas at the
current epoch, the results are encouraging. With some adjustments it may
be possible to obtain a viable model.

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