activity
20052026
most citedProbing the properties of convective cores through g modes: high-order g modes in SPB and gamma Doradus stars

254 citations · 984 across the 25 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.SR2009★ 7 cited

Hybrid gamma Doradus/delta Scuti Stars: Comparison Between Observations and Theory

M. -P. Bouabid, J. Montalban, A. Miglio +3

Gamma Doradus are F-type stars pulsating with high order g-modes. Their instability strip (IS) overlaps the red edge of the delta Scuti one. This observation has led to search for…

astro-ph.SR2009★ 3 cited

The Enigma of B-type Pulsators in the SMC

S. Salmon, J. Montalban, A. Miglio +3

Since the early nineties it is accepted that the excitation mechanism of B-type pulsators on the main sequence is due to the opacity peak in the iron-group elements at $T\approx 20…

astro-ph.SR2009★ 7 cited

Asteroseismology of red-clump stars with CoRoT and Kepler

A. Miglio, J. Montalban, P. Eggenberger +2

The availability of asteroseismic constraints for a large number of red giants with CoRoT and in the near future with Kepler, paves the way for detailed studies of populations of g…

astro-ph.SR2009★ 88 cited

CoRoT's view of newly discovered B-star pulsators: results for 358 candidate B pulsators from the initial run's exoplanet field data

P. Degroote, C. Aerts, M. Ollivier +18

We search for new variable B-type pulsators in the CoRoT data assembled primarily for planet detection, as part of CoRoT's Additional Programme. We aim to explore the properties of…

astro-ph.SR2009★ 31 cited

Ground-based observations of the beta Cephei CoRoT main target HD 180642: abundance analysis and mode identification

M. Briquet, K. Uytterhoeven, T. Morel +20

The known beta Cephei star HD 180642 was observed by the CoRoT satellite in 2007. From the very high-precision light curve, its pulsation frequency spectrum could be derived for th…

astro-ph.SR2009

Testing the forward approach in modelling beta Cephei pulsators: setting the stage

A. Miglio, J. Montalban, A. Thoul

The information on stellar parameters and on the stellar interior we can get by studying pulsating stars depends crucially on the available observational constraints: both seismic…