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- W1618096416 abstract "The angular diameter of a star, combined with observed stellar fluxes in absolute units, allows the absolute fluxes emitted at the surface of the star to be calculated and thus provides a stringent test of model atmosphere predictions. Furthermore, if the flux distribution is observed at all wavelengths contributing significantly to the net flux, an empirical effective temperature can be found. Sufficient data are now available for Sirius (αCMa) to be studied in this way." @default.
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- W1618096416 date "1970-09-01" @default.
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- W1618096416 title "The Absolute Flux Distribution of Sirius" @default.
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- W1618096416 doi "https://doi.org/10.1017/s1323358000012418" @default.
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