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 …
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
Angular momentum transport in stellar interiors
Stars lose a significant amount of angular momentum between birth and death, implying that
efficient processes transporting it from the core to the surface are active. Space …
efficient processes transporting it from the core to the surface are active. Space …
Powering stellar magnetism: energy transfers in cyclic dynamos of Sun-like stars
We use the anelastic spherical harmonic code to model the convective dynamo of solar-type
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …
Asteroseismology of solar-type stars
RA García, J Ballot - Living Reviews in Solar Physics, 2019 - Springer
Until the last few decades, investigations of stellar interiors had been restricted to theoretical
studies only constrained by observations of their global properties and external …
studies only constrained by observations of their global properties and external …
The origin of weakened magnetic braking in old solar analogs
The rotation rates of main-sequence stars slow over time as they gradually lose angular
momentum to their magnetized stellar winds. The rate of angular momentum loss depends …
momentum to their magnetized stellar winds. The rate of angular momentum loss depends …
Convective boundary mixing in main-sequence stars: theory and empirical constraints
EH Anders, MG Pedersen - Galaxies, 2023 - mdpi.com
The convective envelopes of solar-type stars and the convective cores of intermediate-and
high-mass stars share boundaries with stable radiative zones. Through a host of processes …
high-mass stars share boundaries with stable radiative zones. Through a host of processes …
Rotation Periods, Inclinations, and Obliquities of Cool Stars Hosting Directly Imaged Substellar Companions: Spin–Orbit Misalignments Are Common
The orientation between a star's spin axis and a planet's orbital plane provides valuable
information about the system's formation and dynamical history. For non-transiting planets at …
information about the system's formation and dynamical history. For non-transiting planets at …
3D simulations of magnetoconvection in a rapidly rotating supernova progenitor
We present a first 3D magnetohydrodynamic (MHD) simulation of oxygen, neon, and carbon
shell burning in a rapidly rotating core-collapse supernova progenitor. We also run a purely …
shell burning in a rapidly rotating core-collapse supernova progenitor. We also run a purely …
Simulations of solar and stellar dynamos and their theoretical interpretation
We review the state of the art of three dimensional numerical simulations of solar and stellar
dynamos. We summarize fundamental constraints of numerical modelling and the …
dynamos. We summarize fundamental constraints of numerical modelling and the …
Stellar convective penetration: parameterized theory and dynamical simulations
Most stars host convection zones in which heat is transported directly by fluid motion, but the
behavior of convective boundaries is not well-understood. Here, we present 3D numerical …
behavior of convective boundaries is not well-understood. Here, we present 3D numerical …