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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

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