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A role for self-gravity at multiple length scales in the process of star formation

Alyssa A. Goodman, Erik W. Rosolowsky, Michelle A. Borkin, Jonathan B. Foster, Michael Halle, Jens Kauffmann & Jaime E. Pineda

Nature 457, 63-66(1 January 2009)

doi:10.1038/nature07609

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Near-infrared image of the L1448 star-forming region with contours of molecular emission overlaid.

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Figure 2

Comparison of the 'dendrogram' and 'CLUMPFIND' feature-identification algorithms as applied to 13CO emission from the L1448 region of Perseus.

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Figure 3

Schematic illustration of the dendrogram process.

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Figure 4

The fraction of self-gravitating emission as a function of scale in L1448 and a comparable simulation.

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