Stellar winds and molecular outflows

Details Stellar winds and molecular outflows Stellar winds and molecular outflows

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989chphl...6..566m&link_type=abstract

Chinese Physics Letters, Volume 6, Issue 12, pp. 566-569 (1989).

Physics

Scientific paper

We develop a model to explain the high velocities of the ionized stellar winds around young stellar objects associated with magnetic fields. The plasma which is produced by the hot object nearby is turbulent and plays a significant role to accelerate particles. Then the high velocity winds encounter the ambient gas in a molecular cloud to form shock waves. The shocked gas emmision produces broad wings of CO line profiles.

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