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- W27802004 abstract "For the past two years my collaborators and I at the University of Texas at Austin have worked toward establishing an independent distance scale for variable stars. The basis of our approach is to make use of the apparent magnitude and the visual surface brightness, inferred from an appropriate color index, to determine the angular diameter variation of the variable. When combined with the linear displacement curve, obtained from the integrated radial velocity curve, the distance and linear radius are determined. The great attractiveness of the method is its complete independence of all other stellar distance scales. At present a number of practical difficulties exist in implementing the technique, but the results to date are encouraging. In this discussion I will use Cepheid variables to demonstrate the method." @default.
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- W27802004 date "1979-01-01" @default.
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- W27802004 title "An Independent Distance Scale for Variable Stars" @default.
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- W27802004 doi "https://doi.org/10.1017/s025292110007367x" @default.
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