A Multi-Wavelength Study of 30 Doradus Complex in the Large Magellanic Cloud

Details A Multi-Wavelength Study of 30 Doradus Complex in the Large Magellanic Cloud A Multi-Wavelength Study of 30 Doradus Complex in the Large Magellanic Cloud

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jkas...38..365k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 38, no. 3, pp. 365-370

Astronomy and Astrophysics

Astronomy

2

Galaxy: Large Magellanic Cloud, Ism: Atom, Ism: Infrared

Scientific paper

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.

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