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TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems

Astronomy and astrophysics (Berlin), 2020-09, Vol.641, p.A38

Gallet, F.

2020

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Improved angular momentum evolution model for solar-like stars: II. Exploring the mass dependence

Astronomy and astrophysics (Berlin), 2015-05, Vol.577, p.A98

2015

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Improved angular momentum evolution model for solar-like stars

Astronomy and astrophysics (Berlin), 2013-08, Vol.556, p.1-15

2013

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Rotating models of young solar-type stars: Exploring braking laws and angular momentum transport processes

Astronomy and astrophysics (Berlin), 2016-03, Vol.587, p.A105

2016

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Star-planet tidal interaction and the limits of gyrochronology

Astronomy and astrophysics (Berlin), 2019-06, Vol.626, p.A120

2019

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Rotational evolution of solar-type protostars during the star-disk interaction phase

Astronomy and astrophysics (Berlin), 2019-12, Vol.632, p.A6

2019

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Impacts of stellar evolution and dynamics on the habitable zone: The role of rotation and magnetic activity

Astronomy and astrophysics (Berlin), 2017-01, Vol.597, p.A14

2017

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Magnetic field and prominences of the young, solar-like, ultra-rapid rotator V530 Persei

Astronomy and astrophysics (Berlin), 2020-11, Vol.643, p.A39

2020

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The impact of rotation on turbulent tidal friction in stellar and planetary convective regions

Astronomy and astrophysics (Berlin), 2016-08, Vol.592, p.A33

2016

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Monte Carlo simulations of evolving rotational distributions of low-mass stars in young open clusters. Testing the influence of initial conditions

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.510 (1), p.1528-1540

2022

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Disappearance of the extended main sequence turn-off in intermediate age clusters as a consequence of magnetic braking

Astronomy and astrophysics (Berlin), 2019-02, Vol.622, p.A66

2019

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The Fate of Close-in Planets: Tidal or Magnetic Migration?

Astrophysical journal. Letters, 2017-10, Vol.847 (2), p.L16

2017

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Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?

Astronomy and astrophysics (Berlin), 2019-11, Vol.631, p.A111

2019

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Distribution of active forces in the cell cortex

Soft matter, 2019-09, Vol.15 (35), p.6952-6966

2019

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Testing tidal theory for evolved stars by using red giant binaries observed by Kepler

Monthly notices of the Royal Astronomical Society. Letters, 2018-09, Vol.479 (1), p.L123-L128

2018

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Probing active forces via a fluctuation-dissipation relation: Application to living cells

Europhysics letters, 2013-06, Vol.102 (5), p.50005

2013

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Planetary tidal interactions and the rotational evolution of low-mass stars

Astronomy and astrophysics (Berlin), 2018-11, Vol.619

2018

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Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets

Astronomy and astrophysics (Berlin), 2017-08, Vol.604

2017

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First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation

Astronomy and astrophysics (Berlin), 2019-11, Vol.631

2019

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Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets

Astronomy and astrophysics (Berlin), 2017-08, Vol.604

2017

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Planar photonic crystal polarization splitter

Optics letters, 2004-07, Vol.29 (14), p.1620

2004

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Magnetic fields of intermediate-mass T Tauri stars

Astronomy and astrophysics (Berlin), 2019-02, Vol.622

2019

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Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets: I. From the PMS to the RGB at solar metallicity

Astronomy and astrophysics (Berlin), 2017-08, Vol.604, p.A112

2017

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The magnetic strip(s) in the advanced phases of stellar evolution

Astronomy and astrophysics (Berlin), 2017-09, Vol.605

2017

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First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation: From 0.2 to 1.5 M ⊙ at seven metallicities from PMS to TAMS

Astronomy and astrophysics (Berlin), 2019-11, Vol.631, p.A77

2019

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TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems

Improved angular momentum evolution model for solar-like stars: II. Exploring the mass dependence

Improved angular momentum evolution model for solar-like stars

Rotating models of young solar-type stars: Exploring braking laws and angular momentum transport processes

Star-planet tidal interaction and the limits of gyrochronology

Rotational evolution of solar-type protostars during the star-disk interaction phase

Impacts of stellar evolution and dynamics on the habitable zone: The role of rotation and magnetic activity

Magnetic field and prominences of the young, solar-like, ultra-rapid rotator V530 Persei

The impact of rotation on turbulent tidal friction in stellar and planetary convective regions

Monte Carlo simulations of evolving rotational distributions of low-mass stars in young open clusters. Testing the influence of initial conditions

Disappearance of the extended main sequence turn-off in intermediate age clusters as a consequence of magnetic braking

The Fate of Close-in Planets: Tidal or Magnetic Migration?

Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?

Distribution of active forces in the cell cortex

Testing tidal theory for evolved stars by using red giant binaries observed by Kepler

Probing active forces via a fluctuation-dissipation relation: Application to living cells

Planetary tidal interactions and the rotational evolution of low-mass stars

Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets

First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation

Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets

Planar photonic crystal polarization splitter

Magnetic fields of intermediate-mass T Tauri stars

Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets: I. From the PMS to the RGB at solar metallicity

The magnetic strip(s) in the advanced phases of stellar evolution

First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation: From 0.2 to 1.5 M ⊙ at seven metallicities from PMS to TAMS

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