Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-24T01:13:42.519Z Has data issue: false hasContentIssue false
  • English
  • Français

Self-consistent modelling of the dust evolution in damped Ly-alpha systems

Published online by Cambridge University Press:  06 October 2005

E. R. Kasimova  and
Yu. A. Shchekinov
E. R. Kasimova
Affiliation:
Institute of Physics, Rostov University, 194 Stachki Street, Rostov-on-Don, Russia email: [email protected]
Yu. A. Shchekinov
Affiliation:
Department of Physics, Rostov University, 5 Sorge Street, Rostov-on-Don, Russia email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a model which allows for a self-consistent calculation of spectrophotometric, chemical, and dust evolution of spiral and irregular galaxies. Dust evolution is treated without the Instantaneous Recycling Approximation on the basis of the Dwek (1998) model, where up-to-date dust yields for SNe and intermediate mass stars on their AGB phase are taken into account. Confronting model results with the chemical abundances observed in DLA systems, we conclude that spiral and irregular galaxies are good candidates for DLAs.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Colloquium C199: Probing Galaxies through Quasar Absorption Lines , March 2005 , pp. 421 - 423
Copyright
© 2005 International Astronomical Union