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Circumstellar matter, with particular reference to jets and molecular flows

Published online by Cambridge University Press:  04 August 2017

F. D. Kahn
F. D. Kahn*
Affiliation:
Department of Astronomy, University of Manchester, Manchester M13 9PL, England

Abstract

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Circumstellar matter exists in many forms, such as winds from early and from late type stars, in infra-red sources and OH and H2O masers, in X-ray sources and jets, and molecular flows and Herbig-Haro objects. There is considerable diversity in the nature of the starlike bodies that underlie these phenomena. Here an attempt is made to trace the connection between some of the observations related to pre-main sequence stars and their surroundings, with emphasis on jets and molecular flows.

Type
Concluding Remarks
Information
Symposium - International Astronomical Union , Volume 122 , 1987 , pp. 570 - 580
Copyright
Copyright © Reidel 1987