2008/02/29 by Cyrine Nehme, Cyrine Nehmé, J. Le Bourlot +7
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Line (geometry) #Line-of-sight #Molecular cloud #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20078374
10 pages, 17 figures. Accepted for publication in Astronomy and Astrophysics. Typos corrected
openalex publication_date 2008/03/04 · arxiv created 2008/04/03 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We model a diffuse molecular cloud present along the line of sight to the star HD 102065. We compare our modeling with observations to test our understanding of physical conditions and chemistry in diffuse molecular clouds.