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http://dx.doi.org/10.5303/JKAS.2005.38.3.365

A MULTI-WAVELENGTH STUDY OF 30 DORADUS COMPLEX IN THE LARGE MAGELLANIC CLOUD  

Kim, Sung-Eun (Astronomy and Space Science, Sejong University)
Publication Information
Journal of The Korean Astronomical Society / v.38, no.3, 2005 , pp. 365-370 More about this Journal
Abstract
We have made a multi-wavelength study of the X-ray bright giant shell complex 30 Doradus in the Large Magellanic Cloud (LMC). This is the one of the largest H II complexes in the Local Group. The Australia Telescope Compact Array (ATCA) and the Parkes 64-m single dish observations reveal that the distribution and internal motions of H I gas show the effects of fast stellar winds and supernova blasts. The hot emitting gas within the 30 Doradus complex and the entire giant H II complex are encompassed by an expanding H I shell. We investigate the dynamical age of this H I shell and compare to the age of starbursts occurred in the 30 Doradus nebula using the radiative transfer model and the infrared properties.
Keywords
galaxy: Large Magellanic Cloud; ISM: atom; ISM: infrared;
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