Primeval Jets from Young Stars

Details Primeval Jets from Young Stars Primeval Jets from Young Stars

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..241r&link_type=abstract

Highlights of Astronomy, Volume 15, p. 241-242

Astronomy and Astrophysics

Astronomy

Protostar, Yso, Jet, Accretion, Outflow, Herbig-Haro Object, Interstellar Medium

Scientific paper

The jet phenomenon lasts at least a million years for young, solar-like, stars and it occurs during a wide variety of young stellar object (YSO) phases. This includes the period when the source is highly embedded (Class 0) to when it becomes optically visible for the first time as a classical T Tauri star (Class II). Here I briefly discuss some of the properties of jets from the youngest objects.

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