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Analysis of Clumps in Molecular Cloud Models: Mass Spectrum, Shapes, Alignment and Rotation

ASTROPHYSICAL JOURNAL, no. 1 (2003): 203-216

被引用75|浏览8
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Observations reveal concentrations of molecular line emission on the sky, called "clumps," in dense, star-forming molecular clouds. These clumps are believed to be the eventual sites of star formation. We study the three-dimensional analogs of clumps using a set of self-consistent, time-dependent numerical models of molecular clouds. The ...更多

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