Structure and kinematics of molecular jets

Details Structure and kinematics of molecular jets Structure and kinematics of molecular jets

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cajph..64..431s&link_type=abstract

(Conference on Jets from Stars and Galaxies, Toronto, Canada, June 24-27, 1985) Canadian Journal of Physics (ISSN 0008-4204), vo

Astronomy and Astrophysics

Astronomy

Early Stars, Molecular Gases, Radio Jets (Astronomy), Star Formation, Supersonic Jet Flow, Carbon Monoxide, Kinematics, Stellar Mass Ejection

Scientific paper

Observational studies of the structure and kinematics of the supersonic molecular gas in star-forming regions are reviewed. These studies have suggested that the bulk of the high-velocity gas may be ambient-cloud material swept up by a collimated stellar wind. The actual structures of these outflows, however, are poorly understood. One source that may provide a better understanding of molecular outflows is that in the nearby dark cloud LDN 1551. New observations of this outflow are presented and discussed in context of the models proposed by Snell and Schloerb.

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