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WHAT DETERMINES THE DENSITY STRUCTURE OF MOLECULAR CLOUDS? A CASE STUDY OF ORION B WITH HERSCHEL (2013)

First Author: Schneider N

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