C 18 O, 13 CO, and 12 CO abundances and excitation temperatures in the Orion B molecular cloud Analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibrium (2020)
Attributed to:
A Programme of Technology, Astrophysics and Cosmology in Cardiff 2019-22
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202037776
Publication URI: http://dx.doi.org/10.1051/0004-6361/202037776
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics