Population synthesis in stardust galaxies - MKN 710

Details Population synthesis in stardust galaxies - MKN 710 Population synthesis in stardust galaxies - MKN 710

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..131m&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

5

Star Formation, Starburst Galaxies, Milky Way Galaxy, Synthesis

Scientific paper

In the present evolutionary population-synthesis models for the star-formation processes in starburst regions both solar Z and solar Z/10 evolutionary tracks are used to accommodate the general metal deficiency of starburst galaxies. The three parameters synthesized are the Si IV/C IV UV absorption line ratio characterizing the cluster's massive stars, the ratio of the WR(bump) to the H-beta luminosity tracing the WR stars, and the FIR luminosity relating to the extinction due to cluster dust. The stars appear to have formed simultaneously, with a mass spectrum whose slope is in the range (1,2) for massive stars.

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