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Bow shock models of Herbig-Haro objects

Published online by Cambridge University Press:  04 August 2017

A. C. Raga ,
K.-H. Böhm  and
M. Mateo
A. C. Raga
Affiliation:
Astronomy Department, University of Washington, FM-20 Seattle, WA 98195, U.S.A.
K.-H. Böhm
Affiliation:
Astronomy Department, University of Washington, FM-20 Seattle, WA 98195, U.S.A.
M. Mateo
Affiliation:
Astronomy Department, University of Washington, FM-20 Seattle, WA 98195, U.S.A.

Abstract

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It has recently been found that models of a radiating bow shock can explain qualitatively the strange emission line profiles observed in some Herbig-Haro (H-H) objects. It is also possible to compare directly the emission line intensity maps predicted from these models with CCD images of H-H objects. Such a comparison between our models and observations of HH 46/47 is presented, showing that the condensation HH 47A may tentatively be identified with a bow shock formed at the “head” of a jet.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 185 - 186
Copyright
Copyright © Reidel 1987 

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