The Contribution from Circumstellar Dust to the Spectral Energy Distribution of the Large Magellanic Cloud
碩士 === 國立臺灣大學 === 天文物理研究所 === 102 === Unresolved distant galaxies can typically only be studied through their spectral energy distributions (SEDs). An SED model of a galaxy usually con- sists of contributions due to starlight (in the UV/optical and near-infrared) and thermal emission of interstellar...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2013
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| Online Access: | http://ndltd.ncl.edu.tw/handle/73739051187817410339 |