Mass Loss in Young Stellar Objects

Details Mass Loss in Young Stellar Objects Mass Loss in Young Stellar Objects

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..135b&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 1/2, p. 135-144 (1998).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Various aspects of mass loss associated with Young Stellar Objects are reviewed. The classification of the driving sources of the outflows is presented, and the properties of the youngest sources, the Class 0 protostars, are given. The observed properties of the molecular, atomic, and neutral components of the bipolar flows are discussed and critically compared with the most recent theoretical models.

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