Characterising young eclipsing binaries and their environments in NGC 2264
<p>Stellar evolution models underpin much of astrophysics, yet they are severely under-constrained on the pre-main sequence. The masses, radii, temperatures and luminosities of detached double-lined eclipsing binaries (EBs) can be determined in a model-independent manner from the light and rad...
| المؤلفون الرئيسيون: | , |
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| التنسيق: | أطروحة |
| منشور في: |
2015
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