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New Ovro Results Show Disks are Not Necessary for Focussing Bipolar Outflows

Published online by Cambridge University Press:  12 April 2016

M. Barsony
M. Barsony*
Affiliation:
University of California, Berkeley

Extract

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In order to better understand the outflow phenomenon in young, high mass stars, the three sources S87, LkHα101, and S106 were chosen for closer study. High spatial resolution (5” millimeter line 13CO (J=1→0) and CS (J=2→1) maps of these sources were obtained with the Owens Valley Radio Observatory’s (OVRO) millimeter array at 0.15 and 3.0 km s-1 resolutions, respectively.

Type
III. Discs, Outflows, Jets and HH Objects
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 303
Copyright
Copyright © Springer-Verlag 1989