Evolutionary population synthesis in starburst regions

Details Evolutionary population synthesis in starburst regions Evolutionary population synthesis in starburst regions

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...88..399m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 88, no. 3, June 1991, p. 399-450.

Astronomy and Astrophysics

Astrophysics

169

Galactic Evolution, H Ii Regions, Star Formation, Starburst Galaxies, Astronomical Models, Carbon, H Beta Line, Silicon, Spectral Line Width, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature, Wolf-Rayet Stars

Scientific paper

A set of models simulating evolutionary population synthesis was developed using extreme star-formation rates and was used to study the characteristics of several star formation episodes observed in starburst regions. Special attention is given to the effects of different star formation scenarios. Using the synthesized population in combination with a table of mean stellar properties, different observational parameters in the UV, the optical, the FIR, and the radio domains were computed. The evolution of all these parameters during a 20 Myr time period and their sensitivity to the properties of the star formation scenario are examined.

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