The γ Dor stars as revealed by Kepler: A key to reveal deep-layer rotation in A and F stars
EPJ Web of Conferences, 2017 The γ Dor pulsating stars present high-order gravity modes, which make them important targets in the intermediate-and low-mass main-sequence region of the Hertzsprung-Russell diagram. Whilst we have only access to rotation in the envelope of the Sun, the
Salmon S. J. A. J. +4 more
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Chemical element transport in stellar evolution models [PDF]
Royal Society Open Science, 2017 Stellar evolution computations provide the foundation of several methods applied to study the evolutionary properties of stars and stellar populations, both Galactic and extragalactic.
Maurizio Salaris, Santi Cassisi
doaj +1 more source
Three-dimensional hydrodynamics simulations of shell burning in Si/O-rich layer of pre-collapse massive stars [PDF]
EPJ Web of Conferences, 2022 We perform three-dimensional (3D)hydrodynamics simulations of shell burning in the silicon-and oxygen-rich layers in pre-collapse massive stars.Weadoptanon-rotating27 M⊙ starhaving anextended O/Si/Ne layer and afast-rotating 38 M⊙ star having a Si/Olayer,
Yoshida Takashi +7 more
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On compressive radial tidal forces
, 2007 Radial tidal forces can be compressive instead of disruptive, a possibility that is frequently overlooked in high level physics courses. For example, radial tidal compression can emerge in extended stellar systems containing a smaller stellar cluster ...
Binney J. +6 more
core +1 more source
Is there a mass discrepancy in the Cepheid binary OGLE-LMC-CEP0227? [PDF]
, 2011 Context. The Cepheid mass discrepancy, the difference between masses predicted from stellar evolution and stellar pulsation calculations, is a challenge for the understanding of stellar astrophysics. Recent models of the eclipsing binary Cepheid OGLE-LMC-
Bono +36 more
core +1 more source
Stellar Evolution Models of Young Stars: Progress and Limitations
, 2015 Stellar evolution models are a cornerstone of young star astrophysics, which necessitates that they yield accurate and reliable predictions of stellar properties.
Feiden, Gregory A.
core +1 more source
Uncertainties in AGB Evolution and Nucleosynthesis
, 2016 We summarise the evolution and nucleosynthesis in AGB and Super-AGB stars. We then examine the major sources of uncertainty, especially mass-loss.Comment: 8 pages, no figures.
Karakas, Amanda, Lattanzio, John
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Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning [PDF]
, 2014 Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of massive star models computed by different groups each using their own codes, input physics choices and numerical approximations, however, lead to ...
Fryer, C. +7 more
core +2 more sources
Phenomenological Analogies in Black Hole Systems of all Masses
, 2004 I review the progress made on the physics of relativistic jets from black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago.
Mirabel, I. F.
core +2 more sources
Observationally-Motivated Analysis of Simulated Galaxies [PDF]
, 2014 The spatial and temporal relationships between stellar age, kinematics, and chemistry are a fundamental tool for uncovering the physics driving galaxy formation and evolution.
Gibson, B. K. +2 more
core +3 more sources