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Meredith L. Rawls edited figures/KIC11725564_SiB_comparison_1/caption.tex
over 8 years ago
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\label{fig:twin}
Power density spectrum of KIC 11725564 (gray), a seismic ``twin'' of KIC 9246715 (red). Both power spectra are smoothed with a boxcar of $1/10$ of the large separation. The modes in KIC 11725564, a secondary red clump star, have $\Delta \nu$ and $\nu_{\rm{max}}$ which very nearly match KIC 9246715. They are less noisy and have larger amplitudes than
the modes in KIC 9246715, making this star a useful asteroseismic comparison.