58 citations · 110 across the 7 of their papers we have counts for
7 papers
Grids of stellar models with rotation VIII: Models from 1.7 to 500 at metallicity
Yves Sibony, Kendall G. Shepherd, Norhasliza Yusof +12
Grids of stellar evolution models with rotation using the Geneva stellar evolution code (Genec) have been published for a wide range of metallicities. We introduce the last remaini…
A method for non-linear inversion of the stellar structure applied to gravity-mode pulsators
Eoin Farrell, Gaël Buldgen, Georges Meynet +3
We present a method for a non-linear asteroseismic inversion suitable for gravity-mode pulsators and apply it to slowly pulsating B-type (SPB) stars. Our inversion method is based…
Amplitudes of Solar Gravity Modes: A Review
Kévin Belkacem, Charly Pinçon, Gaël Buldgen
Solar gravity modes are considered as the {\it Rosetta Stone} for probing and subsequently deciphering the physical properties of the solar inner-most layers. Recent claims of posi…
Inversions of stellar structure from asteroseismic data
Gaël Buldgen, Jérôme Bétrisey, Ian W. Roxburgh +2
The advent of space-based photometry missions in the early 21st century enabled the application to asteroseismic data of advanced inference techniques until then restricted to the…
Reinvestigating Cen AB in light of asteroseismic forward and inverse methods
Sébastien Salmon, Valérie Van Grootel, Gaël Buldgen +2
The Cen stellar system is the closest neighbour to our Sun. Its main component is a binary composed of two main-sequence stars, one more massive than the Sun and one less massi…
Constraining convective regions with asteroseismic linear structural inversions
G. Buldgen, D. R. Reese, M. A. Dupret
Context. Convective regions in stellar models are always associated with uncertainties, for example due to extra-mixing or the possible inaccurate position of the transition from c…
Determining the metallicity of the solar envelope using seismic inversion techniques
Gaël Buldgen, S. J. A. J. Salmon, A. Noels +3
The solar metallicity issue is a long-lasting problem of astrophysics, impacting multi- ple fields and still subject to debate and uncertainties. While spectroscopy has mostly been…