Astrophysical Laboratories and Advanced Imaging Techniques for Testing Stellar Models: Eclipsing Binaries, High Contrast Imaging, and Optical Interferometry
In chapter 1, we determine the masses, radii and temperatures of the eclipsing binary V578 Mon, a detached system of two early B-type stars in the Rosette Nebula, to better than 5% accuracy. We compare these measurements to the stellar models of the Geneva, Utrecht and Granada group. We find all thr...
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| Format: | Others |
| Language: | en |
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VANDERBILT
2016
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| Online Access: | http://etd.library.vanderbilt.edu/available/etd-04112016-142557/ |