activity
20122024
most citedSeismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

310 citations · 657 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2016★ 136 cited

A new asteroseismic diagnostic for internal rotation in Doradus stars

Rhita-Maria Ouazzani, S. J. A. J. Salmon, V. Antoci +3

With four years of nearly-continuous photometry from Kepler, we are finally in a good position to apply asteroseismology to Doradus stars. In particular several analyses have d…

astro-ph.SR2015★ 63 cited

KIC 10080943: a binary star with two Doradus/ Scuti hybrid pulsators. Analysis of the g modes

M. A. Keen, T. R. Bedding, S. J. Murphy +5

We use four years of Kepler photometry to study the non-eclipsing spectroscopic binary KIC 10080943. We find both components to be Doradus/ Scuti hybrids, which pulsate in b…

astro-ph.SR2012★ 130 cited

Seismic diagnostics for transport of angular momentum in stars 2. Interpreting observed rotational splittings of slowly-rotating red giant stars

M. J. Goupil, B. Mosser, J. P. Marques +4

Asteroseismology with the space-borne missions CoRoT and Kepler provides a powerful mean of testing the modeling of transport processes in stars. Rotational splittings are currentl…

astro-ph.SR2012★ 310 cited

Seismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

J. P. Marques, M. J. Goupil, Y. Lebreton +12

Rotational splittings are currently measured for several main sequence stars and a large number of red giants with the space mission Kepler. This will provide stringent constraints…

astro-ph.SR2012★ 5 cited

Rotational splittings for slow to moderate rotators: Latitudinal dependency or higher order effects in Ω?

R-M. Ouazzani, M-J. Goupil

Information about the rotation rate is contained in the low frequency part of power spectra, where signatures of nonuniform surface rotation are expected, as well as in the frequen…