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PLATO as it is: a legacy mission for Galactic archaeology
A. Miglio, C. Chiappini, B. Mosser +102
Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy.…
Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
Tiago L. Campante, Dimitri Veras, Thomas S. H. North +12
Doppler-based planet surveys point to an increasing occurrence rate of giant planets with stellar mass. Such surveys rely on evolved stars for a sample of intermediate-mass stars (…
A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase
Paola Marigo, Leo Girardi, Alessandro Bressan +13
We introduce a new generation of PARSEC-COLIBRI stellar isochrones that include a detailed treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) phase, and covering a…
Determining stellar parameters of asteroseismic targets: going beyond the use of scaling relations
Thaíse S. Rodrigues, Diego Bossini, Andrea Miglio +6
Asteroseismic parameters allow us to measure the basic stellar properties of field giants observed far across the Galaxy. Most of such determinations are, up to now, based on simpl…
Using red clump stars to correct the Gaia DR1 parallaxes
Guy R. Davies, Mikkel N. Lund, Andrea Miglio +14
Recent results have suggested that there is tension between the Gaia DR1 TGAS distances and the distances obtained using luminosities determined by eclipsing binaries or asteroseis…