Hostname: page-component-76fb5796d-9pm4c Total loading time: 0 Render date: 2024-04-27T02:43:19.582Z Has data issue: false hasContentIssue false
  • English
  • Français

The Collimation of Nonadiabatic Winds from Young Stars

Published online by Cambridge University Press:  12 April 2016

A. C. Raga  and
J. Cantó
A. C. Raga
Affiliation:
Canadian Institute for Theoretical Astrophysics, 60 St. George Street, Toronto, Ontario, Canada
J. Cantó
Affiliation:
Instituto de Astronomía, U.N.A.M. México 20, D. F., México

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Outflows from young stars in many cases show evidence for collimation. For example, bipolar molecular outflows are sometimes quite well collimated (see, e. g., Snell 1982), and stellar jets and Herbig-Haro objects show an even higher degree of collimation (see, e. g., Mundt 1987).

Type
III. Discs, Outflows, Jets and HH Objects
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 276 - 281
Copyright
Copyright © Springer-Verlag 1989

References

Cantó, J. (1980) Astron. Astroph. 86, 327 Google Scholar
Dyson, J. E. 1987. In Circumstellar Matter, IAU Symposium No. 122, edited by Appenzeller, I. and Jordan, C. (Reidel, Dordrecht), p. 159.Google Scholar
Königl, A. 1982, Ap. J. 261, 115.Google Scholar
Mundt, R. 1987. In Circumstellar Matter, IAU Symposium No. 122, edited by Appenzeller, I. and Jordan, C. (Reidel, Dordrecht), p. 147.CrossRefGoogle Scholar
Raga, A. C., and Cantó, J. 1989, Ap. J. (September issue, in press).Google Scholar
Snell, R. 1983, Rev. Mexicana Astron. Astrof. 7, 79.Google Scholar