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Cited article:

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IMPLICATIONS OF RAPID CORE ROTATION IN RED GIANTS FOR INTERNAL ANGULAR MOMENTUM TRANSPORT IN STARS

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TESTING CONVECTIVE-CORE OVERSHOOTING USING PERIOD SPACINGS OF DIPOLE MODES IN RED GIANTS

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ASTEROSEISMIC CLASSIFICATION OF STELLAR POPULATIONS AMONG 13,000 RED GIANTS OBSERVED BY KEPLER

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What asteroseismology can teach us about low-mass core helium burning models

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Non-perturbative effect of rotation on dipolar mixed modes in red giant stars

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Asteroseismology of red giant stars: The potential of dipole modes

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Period-luminosity relations in evolved red giants explained by solar-like oscillations

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Stellar Variability Observed with Kepler

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ASTEROSEISMOLOGY OF THE OPEN CLUSTERS NGC 6791, NGC 6811, AND NGC 6819 FROM 19 MONTHS OFKEPLERPHOTOMETRY

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The mass of the planet-hosting giant starβGeminorum determined from its p-mode oscillation spectrum

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Constraining the core‐rotation rate in red‐giant stars from Kepler space photometry

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Evolutionary influences on the structure of red-giant acoustic oscillation spectra from 600d ofKeplerobservations

T. Kallinger, S. Hekker, B. Mosser, et al.
Astronomy & Astrophysics 541 A51 (2012)
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