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Infrared Classification of Young Stellar Objects
1996The radiative transfer equation for a dusty envelope as close as possible to an embedded central source possesses scaling properties. For a given dust chemical composition, the solution depends only on overall optical depth and the functional form of the radial dust distribution.
Željko Ivezić, Moshe Elitzur
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What Stellar Classification Tells Us
2009When Bunsen and Kirchoff observed the stars spectroscopically, they opened up a new field of observation, and stellar spectroscopy soon became a routine. What the astronomers discovered was a bewildering variety of stellar spectra, to the point of confusion and disarray.
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Quantum-Enhanced Support Vector Machine for Large-Scale Multi-class Stellar Classification
International Conference on Intelligent ComputingKuan-Cheng Chen +4 more
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Classification and Description of Stellar Spectra
1932To Joseph von Fraunhofer we are indebted for the first analyses of the spectra of fixed stars. Though he was concerned with the study of spectra primarily from the standpoint of an optician and maker of achromatic objectives, Fraunhofer’s truly scientific interest led him instinctively to record and describe new phenomena which came under his ...
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Stellar Spectral Classification
2009Richard O. Gray, Christopher J. Corbally
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