EPJ Web of Conferences (Mar 2013)

Differential population studies using asteroseismology: Solar-like oscillating giants in CoRoT fields LRc01 and LRa01

  • Casagrande L.,
  • Baudin F.,
  • Mosser B.,
  • Valentini M.,
  • Noels A.,
  • Montalbán J.,
  • Girardi L.,
  • Chaplin W.J.,
  • Barbieri M.,
  • Morel T.,
  • Chiappini C.,
  • Miglio A.,
  • Fossati L.,
  • Aguirre V. Silva,
  • Baglin A.

DOI
https://doi.org/10.1051/epjconf/20134303004
Journal volume & issue
Vol. 43
p. 03004

Abstract

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Solar-like oscillating giants observed by the space-borne satellites CoRoT and Kepler can be used as key tracers of stellar populations in the Milky Way. When combined with additional photometric/spectroscopic constraints, the pulsation spectra of solar-like oscillating giant stars not only reveal their radii, and hence distances, but also provide well-constrained estimates of their masses, which can be used as proxies for the ages of these evolved stars. In this contribution we provide supplementary material to the comparison we presented in Miglio et al. (2013) between populations of giants observed by CoRoT in the fields designated LRc01 and LRa01.