about
Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modesGravity modes as a way to distinguish between hydrogen- and helium-burning red giant starsHelioseismic measurement of solar torsional oscillations.Ensemble asteroseismology of solar-type stars with the NASA Kepler mission.Hot super-Earths stripped by their host starsDifferential Rotation and Dynamics of the Solar InteriorThe Current State of Solar ModelingHD 181068: a red giant in a triply eclipsing compact hierarchical triple system.Kepler detected gravity-mode period spacings in a red giant starThe Seismic Structure of the SunAccurate Determination of the Solar Photospheric RadiusSolar-like oscillations in the G8 V star τ CetiDoes Kepler unveil the mystery of the Blazhko effect? First detection of period doubling in Kepler Blazhko RR Lyrae starsAsteroseismic modelling of the solar-type subgiant starβ HydriThe non-detection of oscillations in Procyon by MOST: Is it really a surprise?Interferometry and asteroseismology: The radius of τ CetAn ancient extrasolar system with five sub-earth-size planetsHYBRID γ DORADUS-δ SCUTI PULSATORS: NEW INSIGHTS INTO THE PHYSICS OF THE OSCILLATIONS FROMKEPLEROBSERVATIONSTowards a heliological inverse problemSpeed of sound in the solar interiorDifferential asymptotic sound-speed inversionsEffects of diffusion on solar models and their oscillation frequenciesA Bayesian approach to the modelling of α Cen AThe asteroseismic potential of Kepler: first results for solar-type starsThe radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometryThe depth of the solar convection zoneA precise asteroseismic age and radius for the evolved sun-like star KIC 11026764The internal rotation profile of the B-type star KIC 10526294 from frequency inversion of its dipole gravity modesThe PLATO 2.0 missionEstimating the p-mode frequencies of the solar twin 18 ScorpiiPLATO as it is : A legacy mission for Galactic archaeologyABSTRACTSDetection of solar-like oscillations, observational constraints, and stellar models for {theta} Cyg, the brightest star observed by the Kepler missionSpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic dataKOI-3158: The oldest known system of terrestrial-size planetsAsteroseismology of Solar-Type Stars withK2: Detection of Oscillations in C1 DataLimits on surface gravities of Kepler planet-candidate host stars from non-detection of solar-like oscillationsAsteroseismic fundamental properties of solar-type stars observed by the NASA Kepler missionAsteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA array
P50
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P50
description
researcher, ORCID id # 0000-0001-5137-0966
@en
wetenschapper
@nl
name
J. Christensen-Dalsgaard
@nl
Jorgen Christensen-Dalsgaard
@en
Jorgen Christensen-Dalsgaard
@es
type
label
J. Christensen-Dalsgaard
@nl
Jorgen Christensen-Dalsgaard
@en
Jorgen Christensen-Dalsgaard
@es
altLabel
J. Christensen-Dalsgaard
@en
prefLabel
J. Christensen-Dalsgaard
@nl
Jorgen Christensen-Dalsgaard
@en
Jorgen Christensen-Dalsgaard
@es
P106
P21
P31
P496
0000-0001-5137-0966