2006/10/16 by C. Brinch, A. Crapsi, M. R. Hogerheijde +2 · 1 citation
Chemistry · Physics and Astronomy · #Accretion (finance) #Accretion disc #Advanced Physical and Chemical Molecular Interactions #Angular momentum #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Class (philosophy) #Dynamics (music) #Protostar #Star formation #Stellar wind #Young stellar object #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065473
Accepted by A&A, 10 Nov, 2006, 12 pages
openalex publication_date 2006/10/16 · arxiv created 2006/10/23 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context.During protostellar collapse, conservation of angular momentum leads to the formation of an accretion disc. Little is known observationally about how and when the velocity field around the protostar shifts from infall-dominated to rotation-dominated.