Results 61 to 70 of about 5,073 (240)
A calibration of the Rossby number from asteroseismology [PDF]
Astronomy & Astrophysics, 2021 Stellar activity and rotation are tightly related in a dynamo process. Our understanding of this mechanism is mainly limited by our capability of inferring the properties of stellar turbulent convection.
E. Corsaro +6 more
semanticscholar +1 more source
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
TESS Data for Asteroseismology (T’DA) Stellar Variability Classification Pipeline: Setup and Application to the Kepler Q9 Data [PDF]
Astronomical Journal, 2021 The NASA Transiting Exoplanet Survey Satellite (TESS) is observing tens of millions of stars with time spans ranging from ∼27 days to about 1 yr of continuous observations.
J. Audenaert +18 more
semanticscholar +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
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
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 +5 more sources
Pulsating stars harbouring planets
EPJ Web of Conferences, 2013 Why bother with asteroseismology while studying exoplanets? There are several answers to this question. Asteroseismology and exoplanetary sciences have much in common and the synergy between the two opens up new aspects in both fields.
Moya A.
doaj +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 +2 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
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