Journal article
Chemical complexity in high-mass star formation
Abstract
Aims.
In order to understand the observed molecular diversity in high-mass star-forming regions, we have to determine the underlying physical and chemical structure of those regions at high angular resolution and over a range of evolutionary stages.
Authors
Gieser C; Semenov D; Beuther H; Ahmadi A; Mottram JC; Henning T; Beltran M; Maud LT; Bosco F; Leurini S
Journal
Astronomy & Astrophysics, Vol. 631, ,
Publisher
EDP Sciences
Publication Date
11 2019
DOI
10.1051/0004-6361/201935865
ISSN
0004-6361