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Detection of collimated bipolar mass flow in HH24

Published online by Cambridge University Press:  04 August 2017

J. Solf
J. Solf*
Affiliation:
Max-Planck-Institut für Astronomiem Heidelberg

Abstract

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High-resolution long-slit spectroscopy of HH24 has revealed the presence of collimated bipolar mass flow originating from the “central” infrared source SSV63. The bipolar system consists of the well known jet-like HH24C (mean VLSR −190 km s−1 and a newly detected weak component, HH24E (~ + 170 km s−1).

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 191 - 192
Copyright
Copyright © Reidel 1987 

References

Böhm, K. H., Solf, J. 1985, Ap. J. 294, 533.Google Scholar
Herbig, G. H. 1974, Lick Obs. Bull. No. 658.Google Scholar
Solf, J., Böhm, K. H., Raga, A. C. 1986, Ap. J. 305, 795.Google Scholar
Strom, K. M., Strom, S. E., Vrba, F. J. 1976, A. J. 81, 308.Google Scholar