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 2014Show all

13 papers · 1 filter

astro-ph.SR2014★ 35 cited

A search for non-pulsating, chemically normal stars in the Scuti instability strip using Kepler data

Simon J. Murphy, Timothy R. Bedding, Ewa Niemczura +2

We identify stars in the Sct instability strip that do not pulsate in p modes at the 50-mag limit, using Kepler data. Spectral classification and abundance analyses from hig…

astro-ph.SR2014★ 173 cited

Asteroseismic measurement of slow, nearly-uniform surface-to-core rotation in the main sequence F star KIC 9244992

Hideyuki Saio, Donald W. Kurtz, Masao Takata +4

We have found a rotationally split series of core g-mode triplets and surface p-mode multiplets in a main sequence F star, KIC 9244992. Comparison with models shows that the star h…

astro-ph.SR2014★ 28 cited

Echelle diagrams and period spacings of g modes in gamma Doradus stars from four years of Kepler observations

Timothy R. Bedding, Simon J. Murphy, Isabel L. Colman +1

We use photometry from the Kepler Mission to study oscillations in gamma Doradus stars. Some stars show remarkably clear sequences of g modes and we use period echelle diagrams to…

astro-ph.SR2014★ 221 cited

Mixed modes in red giants: a window on stellar evolution

B. Mosser, O. Benomar, K. Belkacem +18

The detection of oscillations with a mixed character in subgiants and red giants allows us to probe the physical conditions in their cores. With these mixed modes, we aim at determ…

astro-ph.EP2014★ 90 cited

Kepler-432: a red giant interacting with one of its two long period giant planets

Samuel N. Quinn, Timothy R. White, David W. Latham +28

We report the discovery of Kepler-432b, a giant planet () transiting an evolved star $(M_\star =…

astro-ph.SR2014★ 93 cited

Non-radial oscillations in M-giant semi-regular variables: Stellar models and Kepler observations

D. Stello, D. Compton, T. R. Bedding +6

The success of asteroseismology relies heavily on our ability to identify the frequency patterns of stellar oscillation modes. For stars like the Sun this is relatively easy becaus…