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The Energy Source of HH34 and its Highly Collimated Jet
Published online by Cambridge University Press: 04 August 2017
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We have discovered a highly collimated optical jet emanating from a faint star and pointing towards the Herbig-Haro object HH34 (Reipurth 1985, Reipurth et al. 1986).
- Type
- I. Star Forming Processes in the Solar Neighborhood
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 396 - 397
- Copyright
- Copyright © Reidel 1987
References
Dyson, J.E.: 1984, in Gas in the Interstellar Medium, ed. Gondhalekar, P.M., Rutherford Appleton Laboratory Workshop, p. 107.Google Scholar
Reipurth, B.: 1985, (Sub)millimeter Astronomy, ESO-IRAM-Onsala workshop, eds. Shaver, P.A. and Kjaer, K., p. 459.Google Scholar
Reipurth, B., Bally, J., Graham, J.A., Lane, A.P., and Zealey, W.J.: 1986, Astron. Astrophys., in press.Google Scholar
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