Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..243k&link_type=abstract
Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at
Astronomy and Astrophysics
Astronomy
2
Scientific paper
Simple numerical considerations show that growth via minor mergers can
be important only for the most massive galaxy disks, and limits to this
process can estimated starting from major-merger rates. A relation is
suggested between the lifetime of dust entering a disk during such
events and the subsequent star-forming history.
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