Models for the evolution of star formation regions in blue compact dwarf galaxies. I - Photometric evolution

Details Models for the evolution of star formation regions in blue compact dwarf galaxies. I - Photometric evolution Models for the evolution of star formation regions in blue compact dwarf galaxies. I - Photometric evolution

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...62p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Mar.-Apr. 1991, p. 62-66. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Dwarf Galaxies, Star Formation, Stellar Evolution, Stellar Models, Blue Stars, H Beta Line, H Ii Regions, Lyman Spectra, Stellar Luminosity

Scientific paper

The photometric characteristics of star formation regions in blue compact dwarf galaxies are considered. Bolometric luminosities, photon fluxes in the Lyman continuum, and the equivalent widths of H-beta emission lines are presented as functions of the age of the star formation region. It is shown that the age of the star formation region is sensitive to the upper limit of the mass of the forming stars.

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