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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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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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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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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

Volltextzugriff (PDF)

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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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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The impact of magnetism on tidal dynamics in the convective envelope of low-mass stars

Proceedings of the International Astronomical Union, 2019-06, Vol.15 (S354), p.195-199

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

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

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

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

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

The impact of magnetism on tidal dynamics in the convective envelope of low-mass stars

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