Determining distances using asteroseismic methods

@article{Aguirre2012DeterminingDU,
  title={Determining distances using asteroseismic methods},
  author={V. Aguirre and L. Casagrande and S. Basu and T. Campante and W. J. Chaplin and D. Huber and A. Miglio and A. Serenelli and Kasc WG1},
  journal={Astronomische Nachrichten},
  year={2012},
  volume={334},
  pages={22-25}
}
  • V. Aguirre, L. Casagrande, +6 authors Kasc WG1
  • Published 2012
  • Physics
  • Astronomische Nachrichten
  • Asteroseismology has been extremely successful in determining the properties of stars in different evolutionary stages with a remarkable level of precision. However, to fully exploit its potential, robust methods for estimating stellar parameters are required and independent verification of the results is needed. In this talk, I present a new technique developed to obtain stellar properties by coupling asteroseismic analysis with the infrared flux method. Using two global seismic observables… CONTINUE READING
    2 Citations

    Figures from this paper.

    References

    SHOWING 1-10 OF 27 REFERENCES
    DETERMINATION OF STELLAR RADII FROM ASTEROSEISMIC DATA
    • 101
    • PDF
    Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array
    • 178
    • Highly Influential
    • PDF
    Constructing a one-solar-mass evolutionary sequence using asteroseismic data from Kepler
    • 51
    • PDF
    Kepler Asteroseismology Program: Introduction and First Results
    • 322
    • PDF
    Accurate fundamental parameters and detailed abundance patterns from spectroscopy of 93 solar-type Kepler targets
    • 160
    • Highly Influential
    • PDF
    Automated extraction of oscillation parameters for Kepler observations of solar-type stars
    • 138
    • PDF
    Asteroseismology of Red Giants as a Tool for Studying Stellar Populations: First Steps
    • 33
    • PDF