Combining two red-giant light curves into unresolved binaries mostly produces low-power, high-entropy power spectra, implying that some complex Kepler stars could be hidden binary systems.
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Power density spectra morphologies of seismically unresolved red-giant asteroseismic binaries
Combining two red-giant light curves into unresolved binaries mostly produces low-power, high-entropy power spectra, implying that some complex Kepler stars could be hidden binary systems.