Title of article
Primeval Jets from Young Stars
Author/Authors
T. P. Ray، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2009
Pages
2
From page
241
To page
242
Abstract
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
protostar , YSO , Jet , outflow , accretion , Interstellar medium , Herbig-Haro object
Journal title
Proceedings of the International Astronomical Union
Serial Year
2009
Journal title
Proceedings of the International Astronomical Union
Record number
674652
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