Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network (2020)
Attributed to:
A Programme of Astrophysics, Cosmology and Technology in Cardiff 2016-19
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Type: Journal Article/Review
Parent Publication: arXiv e-prints