Evolutionary modelling of the M/L ratio for different types of galaxies

Details Evolutionary modelling of the M/L ratio for different types of galaxies Evolutionary modelling of the M/L ratio for different types of galaxies

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61...45s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 45-50) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 27-

Astronomy and Astrophysics

Astronomy

2

Elliptical Galaxies, Galactic Structure, Mass To Light Ratios, Stellar Evolution, Stellar Luminosity, Stellar Mass, Integral Equations, Spectral Energy Distribution, Spiral Galaxies

Scientific paper

The theoretical dependence of the mass-to-luminosity ratio on the initial mass function is obtained for the stellar population of galaxies of different morphological types by evolutionary population synthesis. The evolution of the mass-to-luminosity ratio is calculated for elliptical galaxies. The theoretical dependence of the mass-to-luminosity ratio on the B-V colour for spiral galaxies is compared with empirical data and with other authors' models.

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