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20062026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 4k across the 66 of their papers we have counts for

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Showing 2017Show all

7 papers · 1 filter

astro-ph.SR2017★ 1 cited

Modeling Radial Velocities and Eclipse Photometry of the Kepler Target KIC 4054905: an Oscillating Red Giant in an Eclipsing Binary

M. Benbakoura, P. Gaulme, J. McKeever +3

Asteroseismology is a powerful tool to measure the fundamental properties of stars and probe their interiors. This is particularly efficient for red giants because their modes are…

astro-ph.SR2017★ 78 cited

Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

T. R. White, B. J. S. Pope, V. Antoci +20

The most powerful tests of stellar models come from the brightest stars in the sky, for which complementary techniques, such as astrometry, asteroseismology, spectroscopy, and inte…

astro-ph.SR2017★ 108 cited

Surface rotation of Kepler red giant stars

T. Ceillier, J. Tayar, S. Mathur +7

Kepler allows the measurement of starspot variability in a large sample of field red giants for the first time. With a new method that combines autocorrelation and wavelet decompos…

astro-ph.SR2017★ 26 cited

Evidence for compact binary systems around Kepler red giants

Isabel L. Colman, Daniel Huber, Timothy R. Bedding +9

We present an analysis of 168 oscillating red giants from NASA's mission that exhibit anomalous peaks in their Fourier amplitude spectra. These peaks result from ellipsoid…

astro-ph.SR2017★ 87 cited

Spin alignment of stars in old open clusters

Enrico Corsaro, Yueh-Ning Lee, Rafael A. García +6

Stellar clusters form by gravitational collapse of turbulent molecular clouds, with up to several thousand stars per cluster. They are thought to be the birthplace of most stars an…

astro-ph.EP2017★ 68 cited

Different origins or different evolutions? Decoding the spectral diversity among C-type asteroids

P. Vernazza, J. Castillo-Rogez, P. Beck +15

Anhydrous pyroxene-rich interplanetary dust particles (IDPs) have been proposed as surface analogs for about two-thirds of all C-complex asteroids. However, this suggestion appears…