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An HI Aperture Synthesis Mosaic Survey of the Large Magellanic Cloud

Published online by Cambridge University Press:  25 May 2016

Sungeun Kim ,
L. Staveley-Smith ,
R. J. Sault ,
M. A. Dopita ,
K. C. Freeman ,
M. J. Kesteven  and
D. McConnell
Sungeun Kim
Affiliation:
MSSSO, ANU, Weston Creek PO, Canberra, ACT 2611, Australia
L. Staveley-Smith
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping, NSW 2121, Australia
R. J. Sault
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping, NSW 2121, Australia
M. A. Dopita
Affiliation:
MSSSO, ANU, Weston Creek PO, Canberra, ACT 2611, Australia
K. C. Freeman
Affiliation:
MSSSO, ANU, Weston Creek PO, Canberra, ACT 2611, Australia
M. J. Kesteven
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping, NSW 2121, Australia
D. McConnell
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping, NSW 2121, Australia

Extract

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We present the results of an HI aperture synthesis mosaic of the Large Magellanic Cloud (LMC), made by combining data from 1344 separate pointing centers using the Australia Telescope Compact Array (ATCA). The resolution of the mosaiced image is 1′ (15 pc, using a distance to the LMC of 50 kpc).

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 101 - 102
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Kim, S., Staveley-Smith, L., Dopita, M.A., Freeman, K.C., Sault, R.J., Kesteven, M.J., & McConnell, D. 1998, ApJ, 503, 674.Google Scholar
Kim, S. et al. 1999, in preparation.Google Scholar
Kim, S. 1998, , .Google Scholar