Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.1405s&link_type=abstract
American Astronomical Society Meeting 208, #14.05; Bulletin of the American Astronomical Society, Vol. 38, p.93
Astronomy and Astrophysics
Astronomy
Scientific paper
We report evidence for large amounts of dust around post-starburst K+A galaxies. Using NVO facilities, we searched for circumgalactic dust expected to be produced and ejected by massive starburst galaxies on a timescale of a few 100 Myr. The dust was detected through the extinction and reddening of galaxies in the background of K+A galaxies. We found that the average extinction and reddening in the background of 200 Kpc from the center of a K+A galaxy is 0.3 mag in the g band and 0.1 mag in the g-r color, respectively. This is a surprisingly large amount of extinction, and suggests that mechanisms such as metal-enriched winds and tidal tails are efficient at transporting dust to large radii during galaxy mergers, and that the dust can persist for 1 Gyr if not longer.
Ferguson Harry
Suchkov Anatoly
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