Published in

Cambridge University Press (CUP), Publications of the Astronomical Society of Australia, 1(15), p. 132-135, 1998

DOI: 10.1071/as98132

Links

Tools

Export citation

Search in Google Scholar

HI Supergiant Shells in the Large Magellanic Cloud

Journal article published in 1998 by S. Kim, L. Staveley-Smith ORCID, R. J. Sault, M. J. Kesteven, D. McConnell, M. A. Dopita, M. Bessell ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Green circle
Postprint: archiving allowed
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

Abstract

AbstractThe 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 Hα emission, using a new image taken with a camera lens mounted on the 16-inch telescope at Siding Spring Observatory.

Beta version