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20112026
most citedTight asteroseismic constraints on core overshooting and diffusive mixing in the slowly rotating pulsating B8.3V star KIC 10526294

192 citations · 617 across the 15 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

Effects of Magnetic Fields on Solar Inertial Modes in Global Nonlinear Simulations

Conrado S. Finotti, Gustavo Guerrero, Santiago A. Triana +2

Solar inertial modes are increasingly viewed as probes of the solar interior, with recent helioseismic evidence indicating that these modes may be sensitive to the internal magneti…

astro-ph.SR2025

Simulations of the onset and dynamical evolution of inertial waves in solar/stellar interior

Mariane D. Souza-Gomes, Conrado S. Finotti, Gustavo Guerrero +4

Inertial modes have been recently detected in the Sun via helioseismology, yet their origin, evolution, and role in the dynamics of the solar plasma and magnetic field remain poorl…

astro-ph.SR2022★ 28 cited

Identification of inertial modes in the solar convection zone

Santiago Andrés Triana, Gustavo Guerrero, Ankit Barik +1

The observation of global acoustic waves (p modes) in the Sun has been key to unveiling its internal structure and dynamics. A different kind of wave, known as sectoral Rossby mode…

astro-ph.SR2018

Photometric detection of internal gravity waves in early-type stars observed by CoRoT

D. M. Bowman, C. Aerts, C. Johnston +8

Early-type stars are predicted to excite an entire spectrum of internal gravity waves (IGWs) at the interface of their convective cores and radiative envelopes. Numerical simulatio…

astro-ph.SR2018★ 95 cited

On the photometric detection of Internal Gravity Waves in upper main-sequence stars I. Methodology and application to CoRoT targets

D. M. Bowman, C. Aerts, C. Johnston +8

Context. Main sequence stars with a convective core are predicted to stochastically excite Internal Gravity Waves (IGWs), which effectively transport angular momentum throughout th…

astro-ph.SR2017★ 53 cited

Internal rotation of 13 low-mass low-luminosity red giants in the Kepler field

Santiago Andrés Triana, Enrico Corsaro, Joris De Ridder +3

The Kepler space telescope has provided time series of red giants of such unprecedented quality that a detailed asteroseismic analysis becomes possible. For a limited set of about…

astro-ph.SR2016★ 29 cited

Asteroseismology of 19 low-luminosity red giant stars from Kepler

F. Perez Hernandez, R. A. Garcia, E. Corsaro +2

Frequencies of acoustic and mixed modes in red giant stars are now determined with high precision thanks to the long continuous observations provided by the NASA Kepler mission. He…

astro-ph.SR2015★ 192 cited

Tight asteroseismic constraints on core overshooting and diffusive mixing in the slowly rotating pulsating B8.3V star KIC 10526294

Ehsan Moravveji, Conny Aerts, Peter I. Papics +2

KIC 10526294 is a very slowly rotating and slowly pulsating late B-type star. Its 19 consecutive dipole gravity modes constitute a series with almost constant period spacing. This…