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CO outflows from high-mass Class 0 protostars in Cygnus-X

2013/08/28 by A. Duarte-Cabral, S. Bontemps, F. Motte +4 · 5 citations
Chemistry · Engineering · Physics and Astronomy · #Accretion (finance) #Accretion disc #Astrophysics and Star Formation Studies #Fullerene Chemistry and Applications #Protostar #SAS software applications and methods #Star formation #Stars #T Tauri star #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201321393

Accepted for publication in A&A

openalex publication_date 2013/08/28 · arxiv created 2013/08/29 · arxiv updated 2015/06/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The earliest phases of the formation of high-mass stars are not well known. It is unclear whether high-mass cores in monolithic collapse exist or not, and what the accretion process and origin of the material feeding the precursors of high-mass stars are. As outflows are natural consequences of the accretion process, they represent one of the few (indirect) tracers of accretion.

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