Near-infrared spectroscopy as an astrophysical tool.
Recent improvements in infrared detector arrays make it possible for the first time to conduct detailed spectroscopic studies of a complete range of objects in the 0.9-1.35 μm region. In this dissertation, I examine the 0.9-1.35 μm spectra of planetary and proto-planetary nebulae, M dwarfs, young st...
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| Language: | en |
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The University of Arizona.
1992
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| Online Access: | http://hdl.handle.net/10150/185983 |