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Towards the absolute planes: a new calibration of the bolometric corrections and temperature scales for Population II giants
Authors:P Montegriffo  F R Ferraro  L Origlia  & F Fusi Pecci
Institution:Osservatorio Astronomico di Bologna, Via Zamboni 33, 40126 Bologna, Italy,;Stazione Astronomica, 09012 Capoterra, Cagliari, Italy
Abstract:We present new determinations of bolometric corrections and effective temperature scales as a function of infrared optical colours, using a large data base of photometric observations of about 6500 Population II giants in Galactic globular clusters (GGCs), covering a wide range in metallicity (?2.0 < Fe/H] < 0.0).   New relations for BC K versus ( V  ?  K ) , ( J  ?  K ) and BC V versus ( B  ?  V ), ( V  ?  I ), ( V  ?  J ), and new calibrations for T eff, using both an empirical relation and model atmospheres, are provided.   Moreover, an empirical relation to derive the R parameter of the infrared flux method as a function of the stellar temperature is also presented.
Keywords:techniques: photometric  stars: evolution  stars: fundamental parameters  Hertzsprung–Russell (HR) diagram  stars: Population II  globular clusters: general
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