612 citations · 25.5k across the 406 of their papers we have counts for
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Asteroseismic modelling of the solar-type subgiant star Hydri
I. M. Brandão, G. Dogan, J. Christensen-Dalsgaard +6
Comparing models and data of pulsating stars is a powerful way to understand the stellar structure better.βHyi is an evolved solar-type pulsator with mixed modes in its frequency s…
Asteroseismology of red giants from the first four months of Kepler data: Fundamental parameters
T. Kallinger, B. Mosser, S. Hekker +18
Clear power excess in a frequency range typical for solar-type oscillations in red giants has been detected in more than 1000 stars, which have been observed during the first 138 d…
Asteroseismology of red giants from the first four months of Kepler data: Global oscillation parameters for 800 stars
D. Huber, T. R. Bedding, D. Stello +19
We have studied solar-like oscillations in ~800 red-giant stars using Kepler long-cadence photometry. The sample includes stars ranging in evolution from the lower part of the red-…
A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764
T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson +55
The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-…
Core properties of alpha Cen A using asteroseismology
P. de Meulenaer, F. Carrier, A. Miglio +5
A set of long and nearly continuous observations of alpha Centauri A should allow us to derive an accurate set of asteroseismic constraints to compare to models, and make inference…
Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods
S. Hekker, Y. Elsworth, J. De Ridder +20
The large number of stars for which uninterrupted high-precision photometric timeseries data are being collected with \textit{Kepler} and CoRoT initiated the development of automat…
Period-luminosity relations of pulsating M giants in the solar neighbourhood and the Magellanic Clouds
V. Tabur, T. R. Bedding, L. L. Kiss +3
We analyse the results of a 5.5-yr photometric campaign that monitored 247 southern, semi-regular variables with relatively precise Hipparcos parallaxes to demonstrate an unambiguo…
Solar-like oscillations in cluster stars
D. Stello, S. Basu, T. R. Bedding +21
We present a brief overview of the history of attempts to obtain a clear detection of solar-like oscillations in cluster stars, and discuss the results on the first clear detection…
Asteroseismic modelling of Procyon A: Preliminary results
Gülnur Doğan, Alfio Bonanno, Tim R. Bedding +3
We present our preliminary results of the modelling of the F5 star Procyon A. The frequencies predicted by our models are compared with the frequencies extracted through a global f…
A comparison of Bayesian and Fourier methods for frequency determination in asteroseismology
Timothy R. White, Brendon J. Brewer, Timothy R. Bedding +2
Bayesian methods are becoming more widely used in asteroseismic analysis. In particular, they are being used to determine oscillation frequencies, which are also commonly found by…
Asteroseismology of Solar-type stars with Kepler III. Ground-based Data
Joanna Molenda-Zakowicz, Hans Bruntt, Sergio Sousa +15
We report on the ground-based follow-up program of spectroscopic and photometric observations of solar-like asteroseismic targets for the Kepler space mission. These stars constitu…
Asteroseismology of Solar-type Stars with Kepler I: Data Analysis
C. Karoff, W. J. Chaplin, T. Appourchaux +46
We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5d of scien…
Halo globular clusters observed with AAOmega: dark matter content, metallicity and tidal heating
Richard R. Lane, László L. Kiss, Geraint F. Lewis +6
Globular clusters have proven to be essential to our understanding of many important astrophysical phenomena. Here we analyse spectroscopic observations of ten Halo globular cluste…
A multi-site campaign to measure solar-like oscillations in Procyon. II. Mode frequencies
T. R. Bedding, H. Kjeldsen, T. L. Campante +47
We have analyzed data from a multi-site campaign to observe oscillations in the F5 star Procyon. The data consist of high-precision velocities that we obtained over more than three…
Accurate fundamental parameters for 23 bright solar-type stars
H. Bruntt, T. R. Bedding, P. -O. Quirion +7
We combine results from interferometry, asteroseismology and spectroscopy to determine accurate fundamental parameters of 23 bright solar-type stars, from spectral type F5 to K2 an…
AAOmega Observations of 47 Tucanae: Evidence for a Past Merger?
Richard R. Lane, Brendon J. Brewer, László L. Kiss +6
The globular cluster 47 Tucanae is well studied but it has many characteristics that are unexplained, including a significant rise in the velocity dispersion profile at large radii…
Scaled oscillation frequencies and echelle diagrams as a tool for comparative asteroseismology
Timothy R. Bedding, Hans Kjeldsen
We describe a method for comparing the frequency spectra of oscillating stars. We focus on solar-like oscillations, in which mode frequencies generally follow a regular pattern. On…
Solar-like oscillations in low-luminosity red giants: first results from Kepler
T. R. Bedding, D. Huber, D. Stello +47
We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained w…
The asteroseismic potential of Kepler: first results for solar-type stars
W. J. Chaplin, T. Appourchaux, Y. Elsworth +105
We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal hi…
Discovery of a red giant with solar-like oscillations in an eclipsing binary system from Kepler space-based photometry
S. Hekker, J. Debosscher, D. Huber +26
Oscillating stars in binary systems are among the most interesting stellar laboratories, as these can provide information on the stellar parameters and stellar internal structures.…