Results 1 to 10 of about 328 (203)
The Solar Heavy‐Element Abundances. I. Constraints from Stellar Interiors [PDF]
Astrophysical Journal, 2006 34 pages, 6 figures, Submitted to ...
Marc H Pinsonneault
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A Review of the Mixing Length Theory of Convection in 1D Stellar Modeling
Galaxies, 2023 We review the application of the one-dimensional Mixing Length Theory (MLT) model of convection in stellar interiors and low-mass stellar evolution.
Meridith Joyce, Jamie Tayar
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Rotation rate of the solar core as a key constraint to magnetic angular momentum transport in stellar interiors [PDF]
Astronomy and Astrophysics, 2019 Context. The internal rotation of the Sun constitutes a fundamental constraint when modelling angular momentum transport in stellar interiors. In addition to the more external regions of the solar radiative zone probed by pressure modes, measurements of rotational splittings of gravity modes would offer an invaluable constraint on the rotation of the ...
P Eggenberger +2 more
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Simulations of the Onset and Dynamical Evolution of Inertial Waves in Solar/Stellar Interior
The Astrophysical JournalInertial modes have been recently detected in the Sun via helioseismology, yet their origin, evolution, and role in the dynamics of the solar plasma and magnetic field remain poorly understood.
M. D. Souza-Gomes +6 more
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Magnetism, dynamo action and the solar-stellar connection
Living Reviews in Solar Physics, 2017 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 other phenomena can be uncovered in exquisite detail, but these ...
Allan Sacha Brun, Matthew K. Browning
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Solar-Like Oscillators in the Kepler Era: A Review
Frontiers in Astronomy and Space Sciences, 2021 Many late-type stars across the Milky Way exhibit observable pulsations similar to our Sun that open up a window into stellar interiors. The NASA Kepler mission, a space-based photometric telescope, measured the micro-magnitude luminosity fluctuations ...
Jason Jackiewicz
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News on the slow neutron capture process in AGB stars [PDF]
EPJ Web of Conferences, 2023 Asymptotic giant branch (AGB) stars are responsible for the production of the main component of the solar s-process distribution. Despite enormous progress in the theoretical modeling of these objects over the last few decades, many uncertainties remain.
Vescovi Diego
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Radiative and other effects from internal waves in solar and stellar interiors
Astrophysical Journal, 1981 exaly +2 more sources
The Astrophysical Journal, 2023 We present the first isotopic abundances of both ^13 CO and C ^18 O in solar twin stars and test the results against several galactic chemical evolution (GCE) models with different nucleosynthesis prescriptions.
David R. Coria +5 more
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Ionization potential depression and ionization balance in dense carbon plasma under solar and stellar interior conditions [PDF]
Astronomy & Astrophysics, 2020 Recent quantitative experiments on the ionization potential depression (IPD) in dense plasma show that the observational results are difficult to explain with the widely used analytical models for plasma screening. Here, we investigate the effect of plasma screening on the IPD and ionization balance of dense carbon plasma under solar and stellar ...
Jiaolong Zeng +4 more
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