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Evolution of the star-formation rate and extinction in disk galaxies at high z

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Abstract

A model for the evolution of disk galaxies is used to investigate evolutionary variations in the star-formation rate (SFR) and extinction in disk galaxies beginning from their formation. The results obtained are compared with observational estimates of the SFRe and extinction at cosmological redshifts z ≤ 7. The formof themass-radius relation for disk galaxies is discussed. It is proposed that the mass-radius relation is a consequence of a mass-angular momentum relation. Analysis of the influence of the form of the mass-radius relation on the evolutionary variations in the SFR and extinction testify that this influence is very small. The SFRs and extinctions at various redshifts z obtained in the models are in agreement with observations.

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Authors and Affiliations

  1. Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia

    A. A. Kabanov, A. V. Tutukov & B. M. Shustov

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  1. A. A. Kabanov
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  2. A. V. Tutukov
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  3. B. M. Shustov
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Additional information

Original Russian Text © A.A. Kabanov, A.V. Tutukov, B.M. Shustov, 2011, published in Astronomicheskii Zhurnal, 2011, Vol. 88, No. 3, pp. 218–227.

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Kabanov, A.A., Tutukov, A.V. & Shustov, B.M. Evolution of the star-formation rate and extinction in disk galaxies at high z . Astron. Rep. 55, 193–201 (2011). https://doi.org/10.1134/S1063772911030024

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  • DOI: https://doi.org/10.1134/S1063772911030024

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