Title of article :
Primeval Jets from Young Stars
Author/Authors :
T. P. Ray، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2009
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
Journal title :
Proceedings of the International Astronomical Union