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Implications of the Distribution of HI Clouds in the Lower Galactic Halo

Published online by Cambridge University Press:  17 September 2012

H.A. Ford
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H39, PO Box 218, Hawthorn, Victoria 3122, Australia. e-mail: alyson@astro.swin.edu.au; Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
F.J. Lockman
Affiliation:
National Radio Astronomy Observatory, PO Box 2, Green Bank, WV 24944, USA
N.M. McClure-Griffiths
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
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Abstract

We have detected hundreds of HI clouds in the lower Galactic halo within the Galactic All-Sky Survey pilot region, a region spanning 325l ≤ 343 and |b|≤ 20. The motions of these clouds are governed by Galactic rotation, they are seen within the disk and up to heights of 2.5 kpc, and they span a wide range of Galactocentric radii. However, these clouds are not uniformly distributed and appear to be associated with Galactic structures such as spiral arms or superbubbles.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2012

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