Haboobs in outer space: the when and where of dust storms in distant galaxies
Dust grains are a minor component by mass of the interstellar medium of a galaxy. Yet they can be the dominant source of luminosity. At z ∼ 1, the luminosity density of the Universe in the IR is ∼ 10 times higher than it is at z ∼ 0; common high-redshift galaxies have IR luminosities and dust mass...
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Language: | en_US |
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The University of Arizona.
2014
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Online Access: | http://hdl.handle.net/10150/323445 |