Results 41 to 50 of about 6,468 (258)
On the Detectability of Large-Scale Flows by Asteroseismology
Large-scale convective motions are an integral part of stellar interior dynamics and might play a relevant role in stellar dynamo processes. However, they are difficult to detect or characterize.
Markus Roth, Wiebke Herzberg
doaj +1 more source
Stellar Stalling: the view from asteroseismology [PDF]
Asteroseismology, the study of intrinsic oscillations in stars, can reveal fundamental properties of cool stars critical in our understanding of stellar rotational evolution.
Davies, Guy R. +18 more
core +1 more source
TESS asteroseismology of the Kepler red giants [PDF]
Red giant asteroseismology can provide valuable information for studying the Galaxy as demonstrated by space missions like CoRoT and Kepler. However, previous observations have been limited to small data sets and fields-of-view. The TESS mission provides
D. Stello +13 more
semanticscholar +1 more source
Neutron stars in f(R,T) gravity with conserved energy-momentum tensor: Hydrostatic equilibrium and asteroseismology [PDF]
We investigate the equilibrium and radial stability of spherically symmetric relativistic stars, considering a polytropic equation of state (EoS), within the framework of f(R,T) gravity with a conservative energy-momentum tensor.
J. M. Pretel +3 more
semanticscholar +1 more source
Kepler Asteroseismology Program: Introduction and First Results [PDF]
Asteroseismology involves probing the interiors of stars and quantifying their global properties, such as radius and age, through observations of normal modes of oscillation.
Appourchaux, Thierry +38 more
core +2 more sources
TESS Data for Asteroseismology (T’DA) Stellar Variability Classification Pipeline: Setup and Application to the Kepler Q9 Data [PDF]
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
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
Saturn's Rings as a Seismograph to Probe Saturn's Internal Structure
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 the Nearby K Dwarf σ Draconis Using the Keck Planet Finder and TESS [PDF]
Asteroseismology of dwarf stars cooler than the Sun is very challenging owing to the low amplitudes and rapid timescales of oscillations. Here we present the asteroseismic detection of solar-like oscillations at 4-minute timescales ( νmax∼4300 μHz) in ...
M. Hon +80 more
semanticscholar +1 more source
TESS Data for Asteroseismology: Photometry [PDF]
Over the last two decades, asteroseismology has increasingly proven to be the observational tool of choice for the study of stellar physics, aided by the high quality of data available from space-based missions such as CoRoT, Kepler, K2, and the ...
R. Handberg +13 more
semanticscholar +1 more source

