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The Bolocam Galactic Plane Survey. VII. Characterizing the properties of massive star-forming regions

Dunham, M.K., Rosolowsky, E., Evans Ii, N.J., Cyganowski, C., Urquhart, J.S. (2011) The Bolocam Galactic Plane Survey. VII. Characterizing the properties of massive star-forming regions. Astrophysical Journal, 741 (2). p. 110. ISSN 0004-637X. (doi:10.1088/0004-637X/741/2/110) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:52217)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://dx.doi.org/10.1088/0004-637X/741/2/110
Item Type: Article
DOI/Identification number: 10.1088/0004-637X/741/2/110
Additional information: Unmapped bibliographic data: C7 - 110 [EPrints field already has value set] LA - English [Field not mapped to EPrints] J2 - Astrophys. J. [Field not mapped to EPrints] AD - Department of Astronomy, Yale University, New Haven, CT 06520-8101, United States [Field not mapped to EPrints] AD - Department of Astronomy, University of Texas at Austin, Austin, TX 78712-0259, United States [Field not mapped to EPrints] AD - Department of Physics and Astronomy, University of British Columbia, Okanagan, Kelowna BC V1V 1V7, Canada [Field not mapped to EPrints] AD - Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, United States [Field not mapped to EPrints] AD - CSIRO Astronomy and Space Science, Epping, NSW 1710, Australia [Field not mapped to EPrints] DB - Scopus [Field not mapped to EPrints]
Uncontrolled keywords: dust, extinction, ISM: clouds, ISM: molecules, stars: formation
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User: James Urquhart
Date Deposited: 30 Nov 2015 15:51 UTC
Last Modified: 05 Nov 2024 10:38 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/52217 (The current URI for this page, for reference purposes)

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