Mass outflows from young stellar objects

Details Mass outflows from young stellar objects Mass outflows from young stellar objects

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985comap..10..179s&link_type=abstract

Comments on Modern Physics, Part C - Comments on Astrophysics (ISSN 0146-2970), vol. 10, April 1985, p. 179-186. NASA-NSF-suppor

Astronomy and Astrophysics

Astrophysics

4

Early Stars, Molecular Clouds, Stellar Luminosity, Stellar Mass Ejection, Stellar Winds, Collimation, Mass Flow, T Tauri Stars

Scientific paper

The process of mass loss from young stellar objects is examined in a review of recent observational investigations and theoretical models. Consideration is given to the interaction of the stellar wind with surrounding molecular clouds, the high degree of collimation seen in some embedded objects, alignment of outflows from stars embedded in the same cloud complex, initially isotropic and intrinsically anisotropic models of mass outflow, and the kinds of observations needed to determine the actual mechanisms involved.

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