activity
20102015
most citedGravity modes in rapidly rotating stars. Limits of perturbative methods

80 citations · 183 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20151 cited

A test of the asteroseismic numax scaling relation for solar-like oscillations in main-sequence and sub-giant stars

H. R. Coelho, W. J. Chaplin, S. Basu +3

Large-scale analyses of stellar samples comprised of cool, solar-like oscillators now commonly utilize the so-called asteroseismic scaling relations to estimate fundamental stellar…

astro-ph.SR201435 cited

Stellar acoustic radii, mean densities and ages from seismic inversion techniques

Gaël Buldgen, Daniel Roy Reese, Marc-Antoine Dupret +1

Context. Determining stellar characteristics such as the radius, the mass or the age is crucial when studying stellar evolution, exoplanetary systems or characterising stellar popu…

astro-ph.SR201232 cited

Regular Oscillation Sub-spectrum of Rapidly Rotating Stars

Michael Pasek, François Lignières, Bertrand Georgeot +1

We present an asymptotic theory that describes regular frequency spacings of pressure modes in rapidly rotating stars. We use an asymptotic method based on an approximate solution…

astro-ph.SR201035 cited

On the interpretation of echelle diagrams for solar-like oscillations. Effect of centrifugal distortion

J. C. Suárez, M. J. Goupil, D. R. Reese +4

This work aims at determining the impact of slow to moderate rotation on the regular patterns often present in solar-like oscillation spectra. We focus on the well-known asteroseis…

astro-ph.SR201080 cited

Gravity modes in rapidly rotating stars. Limits of perturbative methods

J. Ballot, F. Lignières, D. R. Reese +1

CoRoT and Kepler missions are now providing high-quality asteroseismic data for a large number of stars. Among intermediate-mass and massive stars, fast rotators are common objects…