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Bow Shocks in Globular Clusters?

Published online by Cambridge University Press:  25 April 2016

D. J. Faulkner  and
Graeme H. Smith
D. J. Faulkner
Affiliation:
Mount Stromlo and Siding Spring Observatories, Private Bag, Weston ACT 2611
Graeme H. Smith
Affiliation:
University of California Observatories & Lick Observatory, University of California, Santa Cruz, USA
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Abstract

It has been suggested that diffuse X-ray sources observed in globular clusters may arise in bow shocks formed by the interaction of intracluster gas with a tenuous halo medium. This paper presents a study both of the cluster space motions and of the energetics of any possible bow shocks which would seem to rule out this hypothesis.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 132 - 134
Copyright
Copyright © Astronomical Society of Australia 1991

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