Physics of Eclipsing Binaries. VI. Hot, Compact Stars
Models of eclipsing binaries require the assignment of appropriate emergent intensities to the surface elements of the binary components. For distance-dependent modeling of flux-calibrated light curves, this necessitates an approximation of the absolute normal intensities of both components of the b...
Kaydedildi:
| Asıl Yazarlar: | , , , , , , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2026-01-01
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| Seri Bilgileri: | The Astrophysical Journal Supplement Series |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-4365/ae844a |
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