Jets and molecular outflows from Herbig-Haro objects

Details Jets and molecular outflows from Herbig-Haro objects Jets and molecular outflows from Herbig-Haro objects

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.311...25s&link_type=abstract

Astrophysics and Space Science, Volume 311, Issue 1-3, pp. 25-34

Astronomy and Astrophysics

Astrophysics

1

Herbig-Haro Objects, Optical Jets, Molecular Outflows, Molecular Jets, X-Winds

Scientific paper

We review status of theoretical development for jets and molecular outflows from young stellar objects. A particular framework for explaining these phenomena is one based on the X-wind theory in an environment of magnetized collapsing molecular cloud cores. The magnetized gravitational collapse follows the standard picture of isolated low-mass star formation, from quasi-static evolution of the parent molecular cloud cores. The outflow phenomena operate throughout the early evolution of young stars as a result of star-disk interaction. We discuss emission mechanisms of jets and formation of molecular outflows in this general framework. The general theoretical framework provides room for self-consistent interpretations for recent observations. Jets and outflows are integral part of earliest evolution of young stellar objects.

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