Importance of source structure on complex organics emission. II: Do disks explain lack of methanol emission from low-mass protostars?

Author(s):
Nazari, P. (0000-0002-4448-3871); Tabone, B.X.J.A.; Rosotti, G.P. (0000-0003-4853-5736); Gelder, M.L. van (0000-0002-6312-8525); Meshaka, R.; Dishoeck, E.F. van (0000-0001-7591-1907)
Published
2022
Publication type
Article / Letter to editor
AstrochemistryStars low-massStars protostarsISM: AbundancesISM moleculesRadiative transferAstrophysics - Solar and Stellar AstrophysicsAstrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A58
hdl
1887/3513595
doi
10.1051/0004-6361/202142777
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...663A..58N