Star formation in molecular disks

Details Star formation in molecular disks Star formation in molecular disks

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98..709p&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Aug. 1986, p. 709-731. Research supported by the Jo

Astronomy and Astrophysics

Astronomy

28

Molecular Clouds, Star Formation, Stellar Evolution, Herbig-Haro Objects, Interstellar Masers, Radio Spectra, Stellar Models, Stellar Spectrophotometry, Stellar Structure

Scientific paper

Recent advances in the observation of star-forming regions have shown that outflows from young stellar objects possess internal structure on scales 1015 - 1017cm, and that molecular disks are seen or suspected to exist around many of these objects. These observations are reviewed and discussed in terms of current theoretical models of wind production and star formation. A variety of observational tests are proposed which are aimed at deciding between the models.

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