Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study on Sh2-201 with JCMT SCUBA-2/POL-2 (2019)
Attributed to:
Astronomy Consolidated Grant at UCLAN
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arXiv.1912.10188
Publication URI: http://dx.doi.org/10.48550/arXiv.1912.10188
Type: Journal Article/Review
Parent Publication: arXiv e-prints