A new starburst model applied to the clumpy irregular galaxy Markarian 325

Details A new starburst model applied to the clumpy irregular galaxy Markarian 325 A new starburst model applied to the clumpy irregular galaxy Markarian 325

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...357...97c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 357, July 1, 1990, p. 97-104. Research supported by NSF and National Natura

Other

154

Astronomical Models, H Ii Regions, Irregular Galaxies, Markarian Galaxies, Starburst Galaxies, Hydrogen Recombinations, Radio Spectra, Stellar Mass, Supernova Remnants, Very Large Array (Vla)

Scientific paper

Radio and far-infrared continuum luminosities, hydrogen recombination-line luminosities, and other data were used to constrain the ionization rate, Type II supernova rate nu(SN), and bolometric luminosity of Mrk 325 and of other starburst galaxies. A new method was used to derive much lower values of nu(SN) from the nonthermal radio luminosity, thereby avoiding the difficulties or contradictions of earlier models. The starburst model provides a quantitative explanation for the observed correlation between the far-infrared and the (mostly nonthermal) radio continuum flux densities of starburst galaxies.

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