AN AMMONIA SPECTRAL MAP OF THE L1495-B218 FILAMENTS IN THE TAURUS MOLECULAR CLOUD. I. PHYSICAL PROPERTIES OF FILAMENTS AND DENSE CORES (2015)

First Author: Seo Y
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/10.1088/0004-637x/805/2/185

Publication URI: http://dx.doi.org/10.1088/0004-637x/805/2/185

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2