Physical properties of dense cores in Orion B9

2010/09/15 by Oskari Miettinen, O. Miettinen, J. Harju +5 · 1 citation
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Computational astrophysics #Interstellar medium #Molecular cloud #Orion Nebula #Phase Equilibria and Thermodynamics #Protostar #Star formation #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201015143

17 pages, 11 figures, 7 tables. Accepted for publication in Astronomy and Astrophysics. Version 2: minor language corrections added

openalex publication_date 2010/09/15 · arxiv created 2010/09/16 · arxiv updated 2015/05/19 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We aim to determine the physical and chemical properties of the starless and protostellar cores in Orion B9, which represents a relatively quiescent star-forming region in Orion B.

Citations

• Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
• The initial core mass function due to ambipolar diffusion in molecular clouds
• The Flattened, Rotating Molecular Gas Core of Protostellar Jet HH 212
• Molecular Evolution in Collapsing Prestellar Cores. III. Contraction of a Bonnor‐Ebert Sphere
• Galactic hydrostatic equilibrium with magnetic tension and cosmic-ray diffusion
• The abundances of nitrogen-containing molecules during pre-protostellar collapse
• Interstellar Ammonia

Cited by

• AHERSCHELAND APEX CENSUS OF THE REDDEST SOURCES IN ORION: SEARCHING FOR THE YOUNGEST PROTOSTARS