HI Supergiant Shells in the Large Magellanic Cloud
S. Kim , L. Staveley-Smith , R.J. Sault , M.J. Kesteven , D. McConnell , M.A. Dopita , M. Bessell, PASA, 15 (1), 132
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HI Supergiant Shells in the Large Magellanic Cloud

S. Kim
L. Staveley-Smith
R.J. Sault
M.J. Kesteven
D. McConnell
M.A. Dopita
M. Bessell

Mount Stromlo and Siding Spring Observatories, Weston Creek PO. ACT 2611, Australia
sek@mso.anu.edu.au
Australia Telescope National Facility, CSIRO, PO Box 76 Epping, NSW 2121, Australia

Abstract:

The recently completed HI mosaic survey of the Large Magellanic Cloud (Kim et al. 1997) reveals complex structure in the interstellar medium including filaments, arcs, holes and shells. We have catalogued giant and supergiant HI shells and searched for correlations with H emission, using a new image taken with a camera lens mounted on the 16-inch Telescope at Siding-Spring Observatory.

Keywords:galaxies:Large Magellanic Cloud - interstellar:HI, H - radio lines: atomic

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