Quantitative inference of the H2 column densities from 3mm molecular emission: case study towards Orion B
Journal article, 2021
methods: statistical
ISM: clouds
ISM: molecules
Author
Pierre Gratier
University of Bordeaux
Jerome Pety
Institut de Radioastronomie Millimétrique (IRAM)
Université Paris PSL
Emeric Bron
Université Paris PSL
Antoine Roueff
Aix Marseille University
Jan Orkisz
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Maryvonne Gerin
Université Paris PSL
Victor de Souza Magalhaes
Institut de Radioastronomie Millimétrique (IRAM)
Mathilde Gaudel
Université Paris PSL
Maxime Vono
University of Toulouse
Sebastien Bardeau
Institut de Radioastronomie Millimétrique (IRAM)
Jocelyn Chanussot
Grenoble Alpes University
Pierre Chainais
University of Lille
Javier R. Goicoechea
CSIC - Instituto de Fisica Fundamental (IFF)
Viviana V. Guzman
Pontificia Universidad Catolica de Chile
Annie Hughes
Paul Sabatier University
Jouni Kainulainen
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
David Languignon
Université Paris PSL
Jacques Le Bourlot
Université Paris PSL
Franck Le Petit
Université Paris PSL
Francois Levrier
Université Paris PSL
Harvey Liszt
National Radio Astronomy Observatory
Nicolas Peretto
Cardiff University
Evelyne Rouefe
Université Paris PSL
Albrecht Sievers
Institut de Radioastronomie Millimétrique (IRAM)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 645 A27Subject Categories
Astronomy, Astrophysics and Cosmology
Atom and Molecular Physics and Optics
Theoretical Chemistry
DOI
10.1051/0004-6361/202037871