Preprint
The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"
Abstract
We use sub-arcsecond resolution ($\sim$0.4$''$) observations with NOEMA at
1.37 mm to study the dust emission and molecular gas of 18 high-mass
Authors
Gieser C; Beuther H; Semenov D; Ahmadi A; Suri S; Möller T; Beltran MT; Klaassen P; Zhang Q; Urquhart JS
Publication date
February 23, 2021
DOI
10.48550/arxiv.2102.11676
Preprint server
arXiv