A MULTI-WAVELENGTH STUDY OF 30 DORADUS COMPLEX IN THE LARGE MAGELLANIC CLOUD |
Kim, Sung-Eun (Astronomy and Space Science, Sejong University) |
1 |
Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud
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DOI |
2 |
Synthesis Imaging in Radio Astronomy
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3 |
The detection of X-ray emission from the OB associations of the Large Magellanic Cloud
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DOI |
4 |
Structure and Evolution of Hot Gas in 30 DOR
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DOI |
5 |
Interstellar bubbles. II - Structure and evolution
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DOI |
6 |
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7 |
An HI Aperture Synthesis Mosaic of the Large Magellanic Cloud
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DOI |
8 |
A Neutral Hydrogen Survey of the Large Magellanic Cloud: Aperture Synthesis and Multibeam Data Combined
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DOI ScienceOn |
9 |
A <TEX>$^{12}CO \; J = 4 {\to}3$</TEX> High-Velocity Cloud in the Large Magellanic Cloud
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DOI ScienceOn |
10 |
Supernova Remnant Candidates in the 30 Doradus Nebula
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DOI |
11 |
A theory of the interstellar medium - Three components regulated by supernova explosions in an inhomogeneous substrate
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DOI |
12 |
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13 |
Kinematic structure of the 30 Doradus giant H II region
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DOI |
14 |
Massive star formation in galaxies: radiative transfer models of the UV to millimetre emission of starburst galaxies
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DOI ScienceOn |
15 |
Opening Address the Magellanic Clouds: DISTANCE, Structure, Chemical Composition
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