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

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

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pgqa.conf..421k&link_type=abstract

Probing Galaxies through Quasar Absorption Lines, IAU Colloquium Proceedings of the International Astronomical Union 199, held M

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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