slides15 - 13 CO J=2-1, integrated over velocity (Sun et...

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Atomic gas Molecular clouds Atomic and molecular gas in the galaxy M33 (Engargiola et al. 2003)
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M51 in CO emission (left) and optical (right) (Koda et al., 2009)
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Pipe Nebula (Lombardi, Alves, & Lada 2006) -- extinction
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The Perseus molecular cloud in
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Unformatted text preview: 13 CO J=2-1, integrated over velocity (Sun et al. 2006) Infrared image of the W5 region from Spitzer The core B68 in a wide variety of tracers. Evolutionary tracks in the HR diagram for stars from 0.6 -6 M . Only lower mass stars have a Hayashi track....
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This note was uploaded on 09/25/2011 for the course ASTRO 112 taught by Professor Krumholz during the Spring '10 term at UCSC.

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slides15 - 13 CO J=2-1, integrated over velocity (Sun et...

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