On the inversion of the Baade-Wesselink technique

Statistics – Computation

Scientific paper

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Cepheid Variables, Computational Astrophysics, Inversions, Stellar Luminosity, Stellar Oscillations, Stellar Temperature, Radii, Stellar Color, Surface Properties

Scientific paper

A general framework is given for the inversion of a 'two-point' formulation of the Baade-Wesselink technique. This means that phases of equal radius are selected and used to get information regarding brightness and temperature. The inversion method is used to evaluate the surface brightness/(V-R) relation in two classical Cepheids, V482 Sco and R TrA. The slope is found to be consistent with previously reported values, but it is argued that the radius determinations will be very uncertain.

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