Results 1 to 10 of about 4,382 (198)
The intermediate neutron capture process
Context. The intermediate neutron-capture process (i-process) can occur during proton ingestion events (PIEs), which may take place in the early evolutionary phases of asymptotic giant branch (AGB) stars. Aims. We investigate the impact of rotational and
Choplin A. +4 more
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Asteroseismology is widely used for the precise mass determination of solar-like oscillating stars, based on individual frequency modeling or homological scaling relations.
Beck P. G. +13 more
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Context. The surface brightness–color relation (SBCR) links stellar color to angular diameter and is a key ingredient of geometric distance measurements on the first rung of the cosmic distance ladder.
Xiong Jianping +7 more
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Rapidly oscillating Ap stars observed with TESS
Context. The rapidly oscillating chemically peculiar A-type (roAp) stars offer valuable insights into the internal physical processes of all stars, but their study is challenged by their rarity. The large-scale Transiting Exoplanet Survey Satellite (TESS)
Rolo Inês +6 more
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Evidence of structural discontinuities in the inner core of red-giant stars. [PDF]
Vrard M +5 more
europepmc +1 more source
The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations. [PDF]
Zhou Y +7 more
europepmc +1 more source
Simulations of Solar and Stellar Dynamos and Their Theoretical Interpretation. [PDF]
Käpylä PJ +4 more
europepmc +1 more source
Variability in the Massive Open Cluster NGC 1817 from K2: A Rich Population of Asteroseismic Red Clump, Eclipsing Binary, and Main-sequence Pulsating Stars. [PDF]
Sandquist EL +15 more
europepmc +1 more source
Editorial: The Future of Asteroseismology
Joyce Ann Guzik, Markus Roth
doaj +1 more source
Gravitational waves from neutron stars and asteroseismology. [PDF]
Ho WCG.
europepmc +1 more source

