2016/11/01 by A. Sanna, L. Moscadelli, R. Cesaroni +4
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Ionization #Jet (fluid) #Mechanics #Momentum (technical analysis) #Momentum transfer #Optics #Outflow #Physics #Star formation #Stars #Stellar, planetary, and galactic studies #Young stellar object #astro-ph.GA #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201629544
5 pages, 2 figures, 2 tables, accepted by Astronomy & Astrophysics
arxiv created 2016/11/01 · openalex publication_date 2016/11/07 · arxiv updated 2016/12/07 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05
Aims. We seek to study the physical properties of the ionized jet emission in the vicinity of an O-type young stellar object (YSO) and to estimate the efficiency of the transfer of energy and momentum from small- to large-scale outflows.