activity
19932026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 25.5k across the 406 of their papers we have counts for

collaborators
Showing 2017Show all

10 papers · 1 filter

astro-ph.SR2017★ 69 cited

Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology

Tanda Li, Timothy R. Bedding, Daniel Huber +4

Stellar models rely on a number of free parameters. High-quality observations of eclipsing binary stars observed by Kepler offer a great opportunity to calibrate model parameters f…

astro-ph.SR2017★ 107 cited

Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries

Simon J. Murphy, Maxwell Moe, Donald W. Kurtz +3

The orbital parameters of binaries at intermediate periods (-- d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new s…

astro-ph.SR2017★ 1 cited

The γ Dor stars as revealed by Kepler : A key to reveal deep-layer rotation in A and F stars

S. J. A. J. Salmon, R. -M. Ouazzani, V. Antoci +2

The γ Dor pulsating stars present high-order gravity modes, which make them important targets in the intermediate-and low-mass main-sequence region of the Hertzsprung-Russell diagr…

astro-ph.EP2017★ 34 cited

Asteroseismic masses of retired planet-hosting A-stars using SONG

D. Stello, D. Huber, F. Grundahl +9

To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars is often difficult.…

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★ 10 cited

Large amplitude change in spot-induced rotational modulation of the Kepler Ap star KIC 2569073

Jason A. Drury, Simon J. Murphy, Aliz Derekas +9

An investigation of the 200 200 pixel 'superstamp' images of the centres of the open clusters NGC 6791 and NGC 6819 allows for the identification and study of many variabl…

astro-ph.SR2017★ 280 cited

Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes

Daniel Huber, Joel Zinn, Mathias Bojsen-Hansen +17

We present a comparison of parallaxes and radii from asteroseismology and Gaia DR1 (TGAS) for 2200 Kepler stars spanning from the main sequence to the red giant branch. We show tha…

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★ 100 cited

First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her

F. Grundahl, M. Fredslund Andersen, J. Christensen-Dalsgaard +26

We report the first asteroseismic results obtained with the Hertzsprung SONG Telescope from an extensive high-precision radial-velocity observing campaign of the subgiant muHerculi…

astro-ph.GA2017★ 6 cited

Stellar population synthesis based modelling of the Milky Way using asteroseismology of dwarfs and subgiants from Kepler

Sanjib Sharma, Dennis Stello, Daniel Huber +2

Early attempts to apply asteroseismology to study the Galaxy have already shown unexpected discrepancies for the mass distribution of stars between the Galactic models and the data…