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Turbulent Mixing Layers in Herbig-Haro and Embedded H2 Jets

Published online by Cambridge University Press:  25 May 2016

Alberto Noriega-Crespo
Alberto Noriega-Crespo*
Affiliation:
Infrared Processing and Analysis Center, California Institute of Technology 100 - 22, Pasadena, California, 91125, USA

Abstract

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Outflows arising from young stellar objects interact with their surrounding medium through different mechanisms, such as shocks, turbulence and /or entrainment. These two last mechanisms have recently begun to be fully developed in an effort to understand the coupling of the stellar jet gas (mostly atomic) with the molecular environment. Observationally a number of objects are being studied in the near infrared and millimeter wavelengths to map the warm (H2) and cold (CO) molecular gas, respectively. In this paper we discuss some of the properties in the near infrared of various embedded jets in the context of turbulent entrainment.

Information

Type
I. Herbig-Haro Objects, H2 Flows and Radio Jets
Information
Symposium - International Astronomical Union , Volume 182: Herbig-Haro Flows and the Birth of Low Mass Stars , 1997 , pp. 103 - 110
Copyright
Copyright © Kluwer 1997 

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