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Observations of jets from young stars

Published online by Cambridge University Press:  04 August 2017

Edward W. Brugel ,
Reinhard Mundt  and
Thomas Bührke
Edward W. Brugel
Affiliation:
Center for Astrophysics and Space Astronomy University of Colorado, Boulder, CO 80309 (USA)
Reinhard Mundt
Affiliation:
Max-Planck Institute for Astronomy Heidelberg, West Germany
Thomas Bührke
Affiliation:
Max-Planck Institute for Astronomy Heidelberg, West Germany

Abstract

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Optical jets, and collimated outflows, are now recognized as a common phenomena associated with young stars (Mundt 1985, Strom et al. 1986). Presented here are the results of new CCD imaging and spatially resolved spectroscopy for ten such objects. Using these and previously published data on twenty known jets, we compiled a set of observational criteria describing the phenomena. From this compilation we addressed several physical questions pertaining to the nature of collimated outflows associated with young stars.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 177 - 178
Copyright
Copyright © Reidel 1987 

References

Brugel, E.W., Böhm, K.H. and Mannery, E. 1981, Ap. J. Sup. 47, 117.CrossRefGoogle Scholar
Mundt, R. 1985 in Protostars and Planets II, eds. Black, D. and Mathews, M., University of Arizona Press, p.414.Google Scholar
Strom, K.M., Strom, S.E., Morgan, J.S., Wolff, S.C., and Wenz, M. 1986 (preprint).Google Scholar