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The Energy Source of HH34 and its Highly Collimated Jet

Published online by Cambridge University Press:  04 August 2017

Bo Reipurth ,
John Bally ,
J. A. Graham ,
A. P. Lane  and
W. J. Zealey
Bo Reipurth
Affiliation:
Copenhagen University Observatory, Øster Voldgade 3, DK-1350 Copenhagen K, Denmark
John Bally
Affiliation:
AT&T Bell Laboratories, Holmdel, New Jersey 07733, USA
J. A. Graham
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, 5241 Broad Branch Road, N.W., Washington, DC 20015, USA
A. P. Lane
Affiliation:
National Radio Astronomy Observatory, Edgemont Road, Charlottesville, Virginia 22901, USA
W. J. Zealey
Affiliation:
Physics Department, University of Wollongong, Wollongong, NSW 2500, Australia

Extract

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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