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Featured researches published by Anne Thoul.


The Astrophysical Journal | 1996

Hydrodynamic simulations of galaxy formation. 2. Photoionization and the formation of low mass galaxies

Anne Thoul; David H. Weinberg

Photoionization by the high-redshift ultraviolet radiation background heats low density gas before it falls into dark matter potential wells, and it eliminates the neutral hydrogen and singly ionized helium that dominate cooling of primordial gas at temperatures of


The Astrophysical Journal | 1994

Element Diffusion in the Solar Interior

Anne Thoul; John N. Bahcall; Abraham Loeb

10^4-10^5


The Astrophysical Journal | 1996

Cosmological formation of low-mass objects

Zoltan Haiman; Anne Thoul; Abraham Loeb

K. We investigate the influence of photoionization on galaxy formation using high-resolution simulations with a 1-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code. We find that the presence of a photoionizing background suppresses the formation of galaxies with circular velocities


Science | 2008

CoRoT measures solar-like oscillations and granulation in stars hotter than the Sun.

Eric Michel; A. Baglin; Michel Auvergne; C. Catala; R. Samadi; F. Baudin; T. Appourchaux; C. Barban; W. W. Weiss; G. Berthomieu; Patrick Boumier; Marc-Antoine Dupret; R. A. García; M. Fridlund; R. Garrido; M. J. Goupil; Hans Kjeldsen; Y. Lebreton; Benoit Mosser; A. Grotsch-Noels; E. Janot-Pacheco; J. Provost; Ian W. Roxburgh; Anne Thoul; Thierry Toutain; Didier Tiphène; Sylvaine Turck-Chieze; Sylvie Vauclair; G. Vauclair; Conny Aerts

v_{circ} \simlt 30\,


Astrophysics and Space Science | 2008

CLÉS, Code Liégeois d'Évolution Stellaire

Richard Scuflaire; S. Théado; J. Montalbán; A. Miglio; P.-O. Bourge; Mélanie Godart; Anne Thoul; A. Noels

\kms\ and substantially reduces the mass of cooled baryons in systems with circular velocities up to


The Astrophysical Journal | 1995

HYDRODYNAMIC SIMULATIONS OF GALAXY FORMATION .1. DISSIPATION AND THE MAXIMUM MASS OF GALAXIES

Anne Thoul; David H. Weinberg

v_{circ} \sim 50\,


Astrophysics and Space Science | 2008

The Liège Oscillation code

Richard Scuflaire; J. Montalbán; S. Théado; P.-O. Bourge; A. Miglio; Mélanie Godart; Anne Thoul; A. Noels

\kms. Above


Monthly Notices of the Royal Astronomical Society | 2007

An asteroseismic study of the β Cephei star θ Ophiuchi: constraints on global stellar parameters and core overshooting

Maryline Briquet; Thierry Morel; Anne Thoul; Richard Scuflaire; A. Miglio; J. Montalbán; M.-A Dupret; Conny Aerts

v_{circ} \sim 75\,


Astronomy and Astrophysics | 2002

Accretion of gas by globular cluster stars

Anne Thoul; Alain Jorissen; Stéphane Goriely; Emmanuel Jehin; Pierre Magain; A. Noels; Geneviève Parmentier

\kms, photoionization has no significant effect. Photoionization exerts its influence primarily by heating gas before collapse; the elimination of line cooling processes is less important. We discuss the implications of these results for hierarchical theories of galaxy formation.


Science | 2009

Solar-Like Oscillations in a Massive Star

K. Belkacem; R. Samadi; M. J. Goupil; Laure Lefevre; F. Baudin; S. Deheuvels; Marc-Antoine Dupret; T. Appourchaux; Richard Scuflaire; Michel Auvergne; C. Catala; Eric Michel; A. Miglio; Josefina Montalban; Anne Thoul; Suzanne Talon; A. Baglin; A. Noels

We study the diffusion of helium and other heavy elements in the solar interior by solving exactly the set of flow equations developed by Burgers for a multi-component fluid, including the residual heat-flow terms. No approximation is made concerning the relative concentrations and no restriction is placed on the number of elements considered. We give improved diffusion velocities for hydrogen, helium, oxygen and iron, in the analytic form derived previously by Bahcall and Loeb. These expressions for the diffusion velocities are simple to program in stellar evolution codes and are expected to be accurate to

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Conny Aerts

Katholieke Universiteit Leuven

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A. Noels

University of Liège

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P. Degroote

Katholieke Universiteit Leuven

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