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Primeval Jets from Young Stars

Published online by Cambridge University Press:  21 October 2010

T. P. Ray
T. P. Ray*
Affiliation:
Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland email: tr@cp.dias.ie
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Abstract

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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.

Keywords

ProtostarYSOjetaccretionoutflowHerbig-Haro objectinterstellar medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 241 - 242
Copyright
Copyright © International Astronomical Union 2010

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