On the inversion of the Baade-Wesselink technique
Author(s) -
Norman R. Simon
Publication year - 1987
Publication title -
publications of the astronomical society of the pacific
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.294
H-Index - 172
eISSN - 1538-3873
pISSN - 0004-6280
DOI - 10.1086/132052
Subject(s) - inversion (geology) , brightness , radius , cepheid variable , physics , surface brightness , astrophysics , geology , optics , computer science , stars , computer security , structural basin , galaxy , paleontology
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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