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

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Showing 2018Show all

10 papers · 1 filter

astro-ph.SR2018★ 22 cited

Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters

Tanda Li, Timothy R. Bedding, Hans Kjeldsen +3

We model the oscillations of the SONG target Herculis to estimate the parameters of the star. The = 1 mixed modes of Her provide strong constraints on stellar proper…

astro-ph.SR2018★ 66 cited

Period spacings of Doradus pulsators in the Kepler field: detection methods and application to 22 slow rotators

Gang Li, Timothy R. Bedding, Simon J. Murphy +3

In Doradus stars, the g-mode period spacing shows an approximately linear relation with period. The slope is a new asteroseismic diagnostic, related to the rotation rate and th…

astro-ph.SR2018★ 24 cited

Surface gravities for 15,000 Kepler stars measured from stellar granulation and validated with Gaia DR2 parallaxes

Durlabh Pande, Timothy R. Bedding, Daniel Huber +1

We have developed a method to estimate surface gravity (log g) from light curves by measuring the granulation background, similar to the "flicker" method by Bastien et al. (2016) b…

astro-ph.GA2018★ 41 cited

The GALAH Survey and Gaia DR2: (Non)existence of five sparse high-latitude open clusters

Janez Kos, Gayandhi de Silva, Joss Bland-Hawthorn +21

Sparse open clusters can be found at high galactic latitudes where loosely populated clusters are more easily detected against the lower stellar background. Because most star forma…

astro-ph.EP2018★ 36 cited

Predicting radial-velocity jitter induced by stellar oscillations based on Kepler data

Jie Yu, Daniel Huber, Timothy R. Bedding +1

Radial-velocity (RV) jitter due to intrinsic stellar variability introduces challenges when characterizing exoplanet systems, particularly when studying small (sub-Neptune-sized) p…

astro-ph.SR2018★ 22 cited

Surface correction of main sequence solar-like oscillators with the LEGACY sample

D. L. Compton, T. R. Bedding, W. H. Ball +4

Poor modelling of the surface regions of solar-like stars causes a systematic discrepancy between the observed and model pulsation frequencies. We aim to characterise this frequenc…

astro-ph.SR2018★ 57 cited

Interferometric diameters of five evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array

T. R. White, D. Huber, A. W. Mann +8

Debate over the planet occurrence rates around intermediate-mass stars has hinged on the accurate determination of masses of evolved stars, and has been exacerbated by a paucity of…

astro-ph.SR2018★ 239 cited

Asteroseismology of 16000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii

Jie Yu, Daniel Huber, Timothy R. Bedding +4

The Kepler mission has provided exquisite data to perform an ensemble asteroseismic analysis on evolved stars. In this work we systematically characterize solar-like oscillations a…

astro-ph.SR2018★ 48 cited

An astrophysical interpretation of the remarkable g-mode frequency groups of the rapidly rotating Dor star, KIC 5608334

H. Saio, T. R. Bedding, D. W. Kurtz +5

The Fourier spectrum of the -Dor variable KIC 5608334 shows remarkable frequency groups at 3, 6, 9, and 11--12\,d. We explain the four frequency groups…

astro-ph.SR2018★ 16 cited

Asteroseismology of KIC 7107778: a binary comprising almost identical subgiants

Yaguang Li, Timothy R. Bedding, Tanda Li +5

We analyze an asteroseismic binary system: KIC 7107778, a non-eclipsing, unresolved target, with solar-like oscillations in both components. We used \emph{Kepler} short cadence tim…