Photometric and chemical evolution of galaxies based on an evolutionary method of population synthesis

Details Photometric and chemical evolution of galaxies based on an evolutionary method of population synthesis Photometric and chemical evolution of galaxies based on an evolutionary method of population synthesis

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...164..260a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 164, no. 2, Aug. 1986, p. 260-273.

Computer Science

Numerical Analysis

208

Astronomical Models, Chemical Evolution, Galactic Evolution, Photometry, Stellar Composition, Metallicity, Numerical Analysis, Star Formation, Star Formation Rate, Stellar Mass

Scientific paper

A program for numerical computations of the photometric and chemical evolution of galaxies is developed. Some initial results are presented suggesting future applications of the program. Each run of model computation has been performed in time steps of 107yr with only the three fundamental parameters of the chemical evolution, i.e., the coefficient ν of star formation rate, the power index μ of initial stellar mass function, and the age TG of the galaxy.

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