Dust layers and molecular flows in young stars

Details Dust layers and molecular flows in young stars Dust layers and molecular flows in young stars

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986s%26w....25..206b&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 25, April 1986, p. 206-210. In German.

Physics

Fluid Dynamics

Early Stars, Molecular Clouds, Molecular Flow, Carbon Monoxide, Dust, Fluid Dynamics, Herbig-Haro Objects, Infrared Astronomy, Milky Way Galaxy, Planetary Systems, Polarimetry

Scientific paper

The observation of dust layers and molecular flows surrounding young stars and their implications for the theory of the formation of stars and planetary systems are discussed. Molecular clouds in the Galaxy and high-velocity CO outflows from them which identify the location of young stars are discussed. The dynamics of the outflows are examined, and the results of infrared polarimetric studies of the outflow regions are reviewed, presenting sample maps.

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