Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array
We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been detected by either Kepler or CoRoT. By combining interferometric angular diameters, Hipparcos parallaxes, asteroseismic densities, bolometric fluxes, and high-resolution spectroscopy, we derive a full set of near-model-independent fundamental...[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Huber_Fundamental_properties_of_2012.pdf||3.8 MB||Adobe PDF|
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