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The HI Supergiant Shells in the Large Magellanic Cloud
1997
International Astronomical Union Colloquium
AbstractWe present the result of an HI aperture synthesis mosaic of the Large Magellanic cloud (LMC), made recently with the Australia Telescope Compact Array (ATCA). The resolution of the mosaiced images is l′.0 (15 pc, using a distance to the LMC of 50 kpc). In contrast to its appearance at other wavelengths, the LMC is remarkably symmetrical in HI on the largest scales, with the bulk of the HI residing in a disk of diameter 8.°4 (7.3 kpc). Outer spiral structure is clearly seen, though the
doi:10.1017/s0252921100071542
fatcat:ei4tsthfkffk7jvspovuirztym