The evolution of the solar wind

AA Vidotto - Living reviews in solar physics, 2021 - Springer
How has the solar wind evolved to reach what it is today? In this review, I discuss the long-
term evolution of the solar wind, including the evolution of observed properties that are …

Magnetism, dynamo action and the solar-stellar connection

AS Brun, MK Browning - Living Reviews in Solar Physics, 2017 - Springer
The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

[HTML][HTML] Binary stars in the new millennium

X Chen, Z Liu, Z Han - Progress in Particle and Nuclear Physics, 2023 - Elsevier
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …

The mass-dependence of angular momentum evolution in Sun-like stars

SP Matt, AS Brun, I Baraffe, J Bouvier… - The Astrophysical …, 2015 - iopscience.iop.org
To better understand the observed distributions of the rotation rate and magnetic activity of
Sun-like and low-mass stars, we derive a physically motivated scaling for the dependence of …

Improved angular momentum evolution model for solar-like stars

F Gallet, J Bouvier - Astronomy & Astrophysics, 2013 - aanda.org
Context. Understanding the origin and evolution of stellar angular momentum is one of the
major challenges of stellar physics. Aims. We present new models for the rotational …

The effect of magnetic topology on thermally driven wind: toward a general formulation of the braking law

V Réville, AS Brun, SP Matt, A Strugarek… - The Astrophysical …, 2015 - iopscience.iop.org
Stellar wind is thought to be the main process responsible for the spin down of main-
sequence stars. The extraction of angular momentum by a magnetized wind has been …

Stellar winds on the main-sequence-II. The evolution of rotation and winds

CP Johnstone, M Güdel, I Brott, T Lüftinger - Astronomy & Astrophysics, 2015 - aanda.org
Aims. We study the evolution of stellar rotation and wind properties for low-mass main-
sequence stars. Our aim is to use rotational evolution models to constrain the mass loss …

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

F Gallet, J Bouvier - Astronomy & Astrophysics, 2015 - aanda.org
Context. Understanding the physical processes that dictate the angular momentum evolution
of solar-type stars from birth to maturity remains a challenge for stellar physics. Aims. We aim …

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

L Amard, A Palacios, C Charbonnel, F Gallet… - Astronomy & …, 2019 - aanda.org
Aims. We present an extended grid of state-of-the art stellar models for low-mass stars
including updated physics (nuclear reaction rates, surface boundary condition, mass-loss …

MHD simulations of accretion onto a dipolar magnetosphere-II. Magnetospheric ejections and stellar spin-down

C Zanni, J Ferreira - Astronomy & Astrophysics, 2013 - aanda.org
Aims. This paper examines the outflows associated with the interaction of a stellar
magnetosphere with an accretion disk. In particular, we investigate the magnetospheric …