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Thermal Radio Jets

Published online by Cambridge University Press:  25 May 2016

Luis F. Rodriguez
Luis F. Rodriguez*
Affiliation:
Instituto de Astronomía, UNAM, Apdo. Postal 70-264, México, DF, 04510 México

Abstract

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Since thermal radio jets can be observed with subarsecond angular resolution and are unaffected by dust absorption, they provide a useful tool to study collimated outflows very close to the young stars that produce them. Here, I review recent results on this area, giving emphasis to the study of thermal jets in the case of the quadrupolar outflows in L723 and HH 111.

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. 83 - 92
Copyright
Copyright © Kluwer 1997 

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