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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)

First Author: Roueff A

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