slides19 - Star formation history for the four regions in...

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QuickTimeª and a decompressor are needed to see this picture. IMF of the Trapezium cluster, a young star cluster (Muench et al. 2002)
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QuickTimeª and a decompressor are needed to see this picture. IMF inferred based on field stars (red) and based on a variety of clusters (blue, green, and black) (Kroupa 2002)
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QuickTimeª and a decompressor are needed to see this picture. Observed HR diagrams (left) in four regions of NGC 2976 (below) (Williams et al. 2009). Contours show observed stars; colored lines show properties for stellar populations 20 Myr - 400 Myr old. QuickTimeª and a decompressor are needed to see this picture.
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QuickTimeª and a decompressor are needed to see this picture. Observed HR diagram (left) and best-fitting model (right) for the OUTER region in NGC 2976.
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Unformatted text preview: Star formation history for the four regions in NGC 2976, showing that, in this galaxy, star formation has occurred more recently in the inner parts than the outer parts of the galaxy. QuickTime and a decompressor are needed to see this picture. Atomic hydrogen distribution (green) and star formation distribution (blue) QuickTime and a decompressor are needed to see this picture. SFR versus atomic gas (left) and molecular gas (right) (Bigiel et al. 2008) QuickTime and a YUV420 codec decompressor are needed to see this picture. QuickTime and a decompressor are needed to see this picture. QuickTime and a decompressor are needed to see this picture. QuickTime and a decompressor are needed to see this picture....
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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 University of California, Santa Cruz.

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slides19 - Star formation history for the four regions in...

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