CO isotopolog line fluxes of viscously evolving disks: cold CO conversion insufficient to explain observed low fluxes

Author(s):
Trapman, L. (0000-0002-8623-9703); Bosman, A.D. (0000-0003-4001-3589); Rosotti, G.P. (0000-0003-4853-5736); Hogerheijde, M.R. (0000-0001-5217-537x); Dishoeck, E.F. van (0000-0001-7591-1907)
Published
2021
Publication type
Article / Letter to editor
Protoplanetary disksAstrochemistryRadiative transferLine: formationAstrophysics - Earth and planetary astrophysicsAstrophysics - solar and stellar astrophysics
Date issued
2021
Language
English
Is part of
Astronomy & Astrophysics (2021), Vol. 649, p. 1-19
hdl
1887/3264040
doi
10.1051/0004-6361/202039200
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...649A..95T