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 …
Pre-supernova outbursts via wave heating in massive stars–I. Red supergiants
J Fuller - Monthly Notices of the Royal Astronomical Society, 2017 - academic.oup.com
Early observations of supernovae (SNe) indicate that enhanced mass-loss and pre-SN
outbursts may occur in progenitors of many types of SNe. We investigate the role of energy …
outbursts may occur in progenitors of many types of SNe. We investigate the role of energy …
A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
I Baraffe, J Clarke, A Morison… - Monthly Notices of …, 2023 - academic.oup.com
We perform two-dimensional (2D) numerical simulations of core convection for zero-age
main-sequence stars covering a mass range from 3 to 20 M⊙. The simulations are …
main-sequence stars covering a mass range from 3 to 20 M⊙. The simulations are …
Photometric detection of internal gravity waves in upper main-sequence stars-II. Combined TESS photometry and high-resolution spectroscopy
Context. Massive stars are predicted to excite internal gravity waves (IGWs) by turbulent core
convection and from turbulent pressure fluctuations in their near-surface layers. These IGWs …
convection and from turbulent pressure fluctuations in their near-surface layers. These IGWs …
A diversity of wave-driven presupernova outbursts
S Wu, J Fuller - The Astrophysical Journal, 2020 - iopscience.iop.org
Many core-collapse supernova (SN) progenitors show indications of enhanced pre-SN mass
loss and outbursts, some of which could be powered by wave energy transport within the …
loss and outbursts, some of which could be powered by wave energy transport within the …
Gravitational wave signals from 3D neutrino hydrodynamics simulations of core-collapse supernovae
H Andresen, B Müller, E Müller… - Monthly Notices of the …, 2017 - academic.oup.com
We present gravitational wave (GW) signal predictions from four 3D multigroup neutrino
hydrodynamics simulations of core-collapse supernovae of progenitors with 11.2, 20 and 27 …
hydrodynamics simulations of core-collapse supernovae of progenitors with 11.2, 20 and 27 …
Internal gravity waves in massive stars: angular momentum transport
We present numerical simulations of internal gravity waves (IGW) in a star with a convective
core and extended radiative envelope. We report on amplitudes, spectra, dissipation, and …
core and extended radiative envelope. We report on amplitudes, spectra, dissipation, and …
Angular momentum transport within evolved low-mass stars
ABSTRACT Asteroseismology of 1.0–2.0 M☉ red giants by the Kepler satellite has enabled
the first definitive measurements of interior rotation in both first ascent red giant branch …
the first definitive measurements of interior rotation in both first ascent red giant branch …
Setting the stage for circumstellar interaction in core-collapse supernovae. II. Wave-driven mass loss in supernova progenitors
JH Shiode, E Quataert - The Astrophysical Journal, 2013 - iopscience.iop.org
SETTING THE STAGE FOR CIRCUMSTELLAR INTERACTION IN CORE-COLLAPSE
SUPERNOVAE. II. WAVE-DRIVEN MASS LOSS IN SUPERNOVA PROGENITORS …
SUPERNOVAE. II. WAVE-DRIVEN MASS LOSS IN SUPERNOVA PROGENITORS …