Interstellar matter and star formation in W5-E

2012/09/05 by L. Deharveng, A. Zavagno, L. D. Anderson +8 · 86 citations
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Dark nebula #Herbig Ae/Be star #Interstellar medium #Molecular cloud #Protostar #Star (game theory) #Star formation #Stellar evolution #Stellar, planetary, and galactic studies #Young stellar object #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201219131

published in Astronomy and Astrophysics 546, A74 (EDP Sciences) · 41 pages, 36 figures, accepted by A&A

openalex publication_date 2012/09/05 · arxiv created 2012/09/13 · arxiv updated 2015/06/11 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We identify the young stellar objects (YSOs) present in the vicinity of the W5-E H ii region, and study the influence of this H ii region on the star formation process in its surrounding molecular material.

Citations

• The NRAO VLA Sky Survey
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• Stellar evolution with rotation

Cited by

• Young Cluster Berkeley 59: Properties, Evolution, and Star Formation
• Kagoshima galactic object survey with the Nobeyama 45-metre telescope by mapping in ammonia lines (KAGONMA): star formation feedback on dense molecular gas in the W33 complex
• From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination withHerschel
• The JCMT Gould Belt Survey: evidence for radiative heating in Serpens MWC 297 and its influence on local star formation