2006/09/20 by H. Jakob, C. Kramer, R. Simon +5 · 1 citation
Chemistry · Physics and Astronomy · #Advanced Physical and Chemical Molecular Interactions #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Carbon monoxide #Energy (signal processing) #Energy budget #Interstellar medium #Molecular cloud #Molecular spectroscopy #Star (game theory) #Star formation #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065855
arxiv created 2006/09/20 · openalex publication_date 2006/10/16 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims. We present an overview of a high-mass star formation region through the major (sub-)mm, and far-infrared cooling lines to gain insight into the physical conditions and the energy budget of the molecular cloud.