This hydrogen cloud is moving away from us at about 330 km/s -- hence its
moniker of a very high velocity cloud. This picture was made from data obtained
as part of the HI Parkes All-Sky Survey. This involves looking for the radio
emissions of concentrations of hydrogen in the local universe. The cloud shown
above covers more of the sky than the Moon and Sun put together, but emits very
little visible light. The green ellipse in the corner of the image shows the
resolution, or beam size, of the telescope, and the green and red parts of the
image are those with the strongest emission. The raw data was reduced and
imaged by David Barnes, Lister Staveley-Smith and Tom Oosterloo.
Click here for a larger version of this image.
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For queries about Melbourne's Astronomy Central contact
Chris Fluke: cfluke@physics.unimelb.edu.au
This page
created on: 16th August, 1997. Last updated: 23rd October, 1997.
Maintained by:
Michael Brown, mbrown@NOSPAM.physics.unimelb.edu.au
Authorised by R.Webster