Journal article
Multi-scale view of star formation in IRAS 21078+5211: from clump fragmentation to disk wind
Abstract
Context.
Star formation (SF) is a multi-scale process in which the mode of fragmentation of the collapsing clump on scales of 0.1–1 pc determines the mass reservoir and affects the accretion process of the individual protostars on scales of 10–100 au.
Authors
Moscadelli L; Beuther H; Ahmadi A; Gieser C; Massi F; Cesaroni R; Sánchez-Monge Á; Bacciotti F; Beltrán MT; Csengeri T
Journal
Astronomy & Astrophysics, Vol. 647, ,
Publisher
EDP Sciences
Publication Date
3 2021
DOI
10.1051/0004-6361/202039837
ISSN
0004-6361