The First Results from the Parkes Multibeam High-Velocity Cloud Survey
arXiv:astro-ph/9902199 · doi:10.1071/AS99070
Abstract
With the onset of the HI Parkes All-Sky Survey, a new view of the high-velocity cloud (HVC) distribution in the southern sky is being revealed. The dense spatial sampling and unbiased coverage of HIPASS gives it multiple advantages over previous surveys of the southern sky. Detailed views of the clouds' structure and large mosaics of the HI sky allow us to link individual concentrations to larger structures (such as the Magellanic Clouds and the Galaxy), providing pictorial clues as to the origins of HVCs. It is clear that HVCs cannot be uniformly assigned a single origin scenario, and must be categorised appropriately.
7 pages with 6 figures in gif format, also available with embedded postscript figures at http://msowww.anu.edu.au/~putman/pubs.html To appear in PASA, vol. 16, no. 1 (Proceedings of "HI in the Local Universe - II)
References in corpus (3)
Cited by in corpus (12)
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- A Very Sensitive 21cm Survey for Galactic High-Velocity HI
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- A blind HI survey in the Canes Venatici region
- High-resolution imaging of compact high-velocity clouds (II)
- Arecibo imaging of compact high-velocity clouds
- A Search for Stellar Populations in High Velocity Clouds
- Detecting Dark Matter in High Velocity Clouds