Constructing a one-solar-mass evolutionary sequence using asteroseismic data from Kepler
Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA Kepler mission, which is providing exquisite data on oscillations of stars across the Hertzsprung-Russell diagram. From the time-series photometry, the two seismic parameters that can be most readily extracted are the large frequency separation (Δν) and the frequency of maximum oscillation power (νmax). After the survey phase, these quantities are available for hundreds of solar-type stars....[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal Letters|
|01_Silva Aguirre_Constructing_a_one-solar-mass_2011.pdf||399.11 kB||Adobe PDF|
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