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An HI Mosaic of the Large Magellanic Cloud

Published online by Cambridge University Press:  05 March 2013

Sungeun Kim ,
K. C. Freeman ,
L. Staveley-Smith ,
R. J. Sault ,
M. J. Kesteven  and
D. McConnell
Sungeun Kim*
Affiliation:
Mount Stromlo & Siding Spring Observatories, Private Bag, Weston ACT 2611, Australia
K. C. Freeman
Affiliation:
Mount Stromlo & Siding Spring Observatories, Private Bag, Weston ACT 2611, Australia
L. Staveley-Smith
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia.
R. J. Sault
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia.
M. J. Kesteven
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia.
D. McConnell
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia.
*
[email protected]
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Abstract

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The parameters of a new Australia Telescope Compact Array (ATCA) mosaic of the Large Magellanic Cloud (LMC) in the 21-cm line of neutral hydrogen are described. A preliminary peak-brightness-temperature image of the whole of the LMC, and a detailed image of the region around the supergiant shells LMC 4 and 5 is shown.

Type
Hi in the Local Universe
Information
Publications of the Astronomical Society of Australia , Volume 14 , Issue 1 , 1997 , pp. 119 - 121
Copyright
Copyright © Astronomical Society of Australia 1997

References

de Vaucouleurs, G., & Freeman, K. C. 1972, Vistas in Astronomy, 14, 163 Google Scholar
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