From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination withHerschel

2015/09/21 by P. Didelon, F. Motte, P. Tremblin +39
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Computational astrophysics #Envelope (radar) #Gravitational collapse #H II region #Molecular cloud #Scientific Research and Discoveries #astro-ph.GA #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201526239

published as A&A 584, A4 (2015) · 25pages A&A sous presse

openalex publication_date 2015/09/21 · arxiv created 2015/10/30 · arxiv updated 2015/11/25 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The surroundings of H ii regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H ii regions in the MonR2 molecular cloud.

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