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Buldgen, G.
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Buldgen, G.
Buldgen, Gaël
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gbuldgen@student.ulg.ac.be
gael.buldgen@unige.ch
Gael.Buldgen@unige.ch
G.Buldgen@bham.ac.uk
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http://hub.abes.fr/edp/periodical/aa/2015/volume_574/issue_2015/aa24613-14/authorship/1
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Stellar acoustic radii, mean densities, and ages from seismic inversion techniques
Constraints on the structure of 16 Cygni A and 16 Cygni B using inversion techniques
Seismic solar models from Ledoux discriminant inversions
Thorough characterisation of the 16 Cygni system
Reinvestigating α Centauri AB in light of asteroseismic forward and inverse methods
Convective core sizes in rotating massive stars
Star-planet interactions
Standard solar models: Perspectives from updated solar neutrino fluxes and gravity-mode period spacing
Grids of stellar models with rotation
The key impact of the host star’s rotational history on the evolution of TOI-849b
CORALIE radial-velocity search for companions around evolved stars (CASCADES)
CORALIE radial velocity search for companions around evolved stars (CASCADES)
CORALIE radial-velocity search for companions around evolved stars (CASCADES)
Kepler-93: A testbed for detailed seismic modelling and orbital evolution of super-Earths around solar-like stars
Asteroseismology of β Cephei stars: The stellar inferences tested in hare and hound exercises
Thorough characterisation of the 16 Cygni system
Probing stellar cores from inversions of frequency separation ratios
Backtracing the internal rotation history of the β Cep star HD 129929
Evidence of a signature of planet formation processes from solar neutrino fluxes
Constraints on planetary tidal dissipation from a detailed study of Kepler 91b
Higher metal abundances do not solve the solar problem
Using seismic inversions to obtain an indicator of internal mixing processes in main-sequence solar-like stars
In-depth study of 16CygB using inversion techniques
SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
Constraining convective regions with asteroseismic linear structural inversions
Asteroseismology of evolved stars to constrain the internal transport of angular momentum
Combining multiple structural inversions to constrain the solar modelling problem
Comprehensive stellar seismic analysis
Rotation rate of the solar core as a key constraint to magnetic angular momentum transport in stellar interiors
Revisiting Kepler-444
Asteroseismology of evolved stars to constrain the internal transport of angular momentum
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