Results 61 to 70 of about 14,588 (266)
Constraining stellar evolution theory with asteroseismology of γ Doradus stars using deep learning [PDF]
Astronomy & Astrophysics, 2021 Context. The efficiency of the transport of angular momentum and chemical elements inside intermediate-mass stars lacks proper calibration, thereby introducing uncertainties on a star’s evolutionary pathway.
J. Mombarg, T. V. Reeth, C. Aerts
semanticscholar +1 more source
Physics Today, 2015 Pulsations known as starquakes can provide precious glimpses into a star’s interior—and clues to how the star will live and die.
openaire +3 more sources
The Current Status of Asteroseismology [PDF]
Solar Physics, 2008 20 pages, 5 figures, accepted for publication in Solar ...
Conny Aerts +4 more
openaire +7 more sources
White Dwarfs as Physics Laboratories: Lights and Shadows
Frontiers in Astronomy and Space Sciences, 2022 The evolution of white dwarfs is essentially a gravothermal process of cooling in which the basic ingredients for predicting their evolution are well identified, although not always well understood. There are two independent ways to test the cooling rate.
J. Isern +6 more
doaj +1 more source
Saturn's Rings as a Seismograph to Probe Saturn's Internal Structure
AGU Advances, Volume 1, Issue 2, June 2020., 2020 As it has already done for Earth, the Sun, and the stars, seismology has the potential to radically change the way the interiors of giant planets are studied. In a sequence of events foreseen by only a few, observations of Saturn's rings by the Cassini spacecraft have rapidly broken ground on giant planet seismology. Gravity directly couples the planet'
Christopher R. Mankovich
wiley +1 more source
Asteroseismology of Procyon with SOPHIE [PDF]
Astronomy & Astrophysics, 2007 This paper reports a 9-night asteroseismic observation program conducted in January 2007 with the new spectrometer Sophie at the OHP 193-cm telescope, on the F5 IV-V target Procyon A. This first asteroseismic program with Sophie was intended to test the performance of the instrument with a bright but demanding asteroseismic target and was part of a ...
Mosser, B. +11 more
openaire +7 more sources
Radial Oscillations in Neutron Stars from Unified Hadronic and Quarkyonic Equation of States
Galaxies, 2023 We study radial oscillations in non-rotating neutron stars by considering the unified equation of states (EoSs), which support the 2 M⊙ star criterion.
Souhardya Sen +7 more
doaj +1 more source
Gravitational wave asteroseismology of dark matter hadronic stars [PDF]
Physical Review DThe influence of the dark matter mass~($M_{\chi}$) and the Fermi momentum~($k_{F}^{\dm}$) on the $f_0$-mode oscillation frequency, damping time parameter, and tidal deformability of hadronic stars are studied by employing a numerical integration of ...
César V. Flores +4 more
semanticscholar +1 more source
Asteroseismology of solar-type stars [PDF]
Living Reviews in Solar Physics, 2019 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 characteristics.
R. García, J. Ballot
semanticscholar +1 more source
TESS Data for Asteroseismology: Light-curve Systematics Correction [PDF]
Astrophysical Journal Supplement Series, 2021 Data from the Transiting Exoplanet Survey Satellite (TESS) have produced of the order of one million light curves at cadences of 120 s and especially 1800 s for every ∼27 day observing sector during its two-year nominal mission.
M. Lund +8 more
semanticscholar +1 more source