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20182025
most citedThorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd

25 citations · 134 across the 14 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2025★ 4 cited

The theoretical pulsation spectra of hot B subdwarfs. Static and evolutionary STELUM models

N. Guyot, V. Van Grootel, S. Charpinet +3

Context. The Kepler and TESS space missions have revealed the rich gravity (g-)mode pulsation spectra of many hot subdwarf B (sdB) stars in detail. These spectra exhibit complex be…

astro-ph.SR2025

Detailed seismic study of Gemma (KIC11026764) using EGGMiMoSA: Unveiling the probing potential of mixed modes for subgiant stars

M. Farnir, M. -A. Dupret, G. Buldgen

Context. When leaving the main sequence (MS) for the red-giant branch (RGB), subgiant stars undergo fast structural changes. Consequently, their observed oscillation spectra mirror…

astro-ph.SR2024

MCMC inversions of the internal rotation of Kepler subgiants

G. Buldgen, L. Fellay, J. Bétrisey +3

The measurement of the internal rotation of post-main sequence stars using data from space-based photometry missions has demonstrated the need for an efficient angular momentum tra…

astro-ph.SR2023★ 11 cited

Asteroseismic modelling strategies in the PLATO era I. Mean density inversions and direct treatment of the seismic information

Jérôme Bétrisey, Gaël Buldgen, Daniel R. Reese +6

Asteroseismic modelling will be part of the pipeline of the PLATO mission and will play a key role in the mission precision requirements on stellar mass, radius and age. It is ther…

astro-ph.SR2023★ 3 cited

Study with WhoSGlAd of the acoustic depth of the helium glitch across the seismic HR diagram and its impact on the inferred helium abundance

Martin Farnir, Angelo Valentino, Marc-Antoine Dupret +1

The acoustic glitches' signature present in solar-like stars holds invaluable information. Indeed, it is caused by a sharp variation in the sound speed, therefore carrying localise…

astro-ph.SR2022★ 17 cited

Thorough characterisation of the 16 Cygni system. Part II. Seismic inversions of the internal structure

G. Buldgen, M. Farnir, P. Eggenberger +5

The advent of space-based photometry observations provided high-quality asteroseismic data for a large number of stars. These observations enabled the adaptation of advanced techni…

astro-ph.SR2022★ 14 cited

Apsidal motion in massive eccentric binaries in NGC 6231: The case of HD 152219

S. Rosu, G. Rauw, M. Farnir +2

The measurement of the apsidal motion in close eccentric massive binary systems provides essential information to probe the internal structure of the stars that compose the system.…

astro-ph.SR2021★ 9 cited

Asteroseismology of evolved stars with EGGMiMoSA I. Theoretical mixed-mode patterns from the subgiant to the RGB phase

M. Farnir, C. Pinçon, M-A. Dupret +2

This study is the first of a series of papers that provide a technique to analyse the mixed-modes frequency spectra and characterise the structure of stars on the subgiant and red-…

astro-ph.SR2020★ 25 cited

Thorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd

M. Farnir, M. -A. Dupret, G. Buldgen +5

Context: Being part of the brightest solar-like stars, and close solar analogues, the 16 Cygni system is of great interest to the scientific community and may provide insight into…

astro-ph.SR2020★ 21 cited

Apsidal motion in the massive binary HD 152248 -- Constraining the internal structure of the stars

S. Rosu, A. Noels, M. -A. Dupret +3

Apsidal motion in massive eccentric binaries offers precious information about the internal structure of the stars. This is especially true for twin binaries consisting of two near…

astro-ph.SR2019

From the Sun to solar-like stars: how does the solar modelling problem affect our studies of solar-like oscillators?

G. Buldgen, C. Pezzotti, M. Farnir +2

Since the first observations of solar oscillations in 1962, helioseismology has probably been one of the most successful fields of astrophysics. Besides the improvement of observat…

astro-ph.SR2019

Comprehensive stellar seismic analysis: A preliminary application of Whosglad to 16 Cygni system

M. Farnir, M-A. Dupret, S. J. A. J. Salmon +2

We present a first application of Whosglad method to the components A and B of the 16 Cygni system. The method was developed to provide a comprehensive analysis of stellar oscillat…

astro-ph.SR2019★ 4 cited

Revisiting Kepler-444 Part I. Seismic modelling and inversions of stellar structure

G. Buldgen, M. Farnir, C. Pezzotti +10

Context. The CoRoT and Kepler missions have paved the way for synergies between exoplanetology and asteroseismology. The use of seismic data helps providing stringent constraints o…

astro-ph.SR2018★ 20 cited

Comprehensive stellar seismic analysis : New method exploiting the glitches information in solar-like pulsators

M. Farnir, M-A. Dupret, S. J. A. J. Salmon +2

Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar-like pulsators. We define new seismic indicators that should be as uncorrelated…