WHAT DETERMINES THE DENSITY STRUCTURE OF MOLECULAR CLOUDS? A CASE STUDY OF ORION B WITH HERSCHEL (2013)
Attributed to:
Pre-stellar and protostellar core evolution with Herschel, SCUBA2 and ALMA.
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/2041-8205/766/2/l17
Publication URI: http://dx.doi.org/10.1088/2041-8205/766/2/l17
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 2041-8205