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 Hα emission, using a new image taken with a camera lens mounted on the 16-inch telescope at Siding Spring Observatory.
Author supplied keywords
Cite
CITATION STYLE
APA
Kim, S., Staveley-Smith, L., Sault, R. J., Kesteven, M. J., McConnell, D., Dopita, M. A., & Bessell, M. (1998). HI supergiant shells in the large magellanic cloud. Publications of the Astronomical Society of Australia, 15(1), 132–135. https://doi.org/10.1071/AS98132
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free