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Molecular Studies of Herbig-Haro Objects

Published online by Cambridge University Press:  07 August 2017

Salvador Curiel
Salvador Curiel*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street (MS 10) Cambridge, MA 02138

Abstract

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Recent ultraviolet, infrared, millimeter and centimeter-wavelength observations have revealed that HH objects are also sources of molecular line emission. Infrared observations have shown that H2 line emission in HH objects presents a wide and complex variety of morphologies, being in most of the cases similar to that observed at optical wavelengths. New high-angular resolution radio observations of molecular lines have revealed that small high-density condensations are frequently found in association with HH objects. Below, a brief review of molecular emission in HH objects is presented.

Type
Near Stellar Environments
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 373 - 378
Copyright
Copyright © Kluwer 1992 

References

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