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- W1630773996 abstract "Context. The eclipsing binary method for determining distance in the local group is based on the surface brightness-color relation (SBCR), and early-type stars are preferred targets because of their intrinsic brightness. However, this type of star exhibits wind, mass-loss, pulsation, and rotation, which may generate bias on the angular diameter determination. An accurate calibration of the SBCR relation thus requires careful analysis." @default.
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- W1630773996 date "2015-07-01" @default.
- W1630773996 modified "2023-10-17" @default.
- W1630773996 title "Theoretical impact of fast rotation on calibrating the surface brightness-color relation for early-type stars" @default.
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- W1630773996 doi "https://doi.org/10.1051/0004-6361/201526240" @default.
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