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Cited by 241

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STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS

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Evans, Neal J., Heiderman, Amanda, Vutisalchavakul, Nalin·2014·The Astrophysical Journal

Abstract

We test some ideas for star formation relations against data on local molecular clouds. On a cloud by cloud basis, the relation between the surface density of star formation rate and surface density of gas divided by a free-fall time, calculated from the mean cloud density, shows no significant correlation. If a crossing time is substituted for the free-fall time, there is even less correlation. Within a cloud, the star formation rate volume and surface densities increase rapidly with the corresponding gas densities, faster than predicted by models using the free-fall time defined from the local density. A model in which the star formation rate depends linearly on the mass of gas above a visual extinction of 8 mag describes the data on these clouds, with very low dispersion. The data on regions of very massive star formation, with improved star formation rates based on free–free emission from ionized gas, also agree with this linear relation.

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Crossref · 10.1088/0004-637x/782/2/114

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Metadata

Authors
Evans, N. J., Heiderman, A., & Vutisalchavakul, N.
Venue
The Astrophysical Journal
Published
2014-02-04
Volume
782
Issue
2
Pages
114
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2037247549
Cited by
241
References
3
FWCI
12.91
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS. https://app.cochat.ai/papers/10.1088/0004-637x/782/2/114
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Evans, N. J., Heiderman, A., & Vutisalchavakul, N. (2014). STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/782/2/114

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