Fundamental properties of Kepler planet-candidate host stars using asteroseismology
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Ages and fundamental properties of Kepler exoplanet host stars from asteroseismologyOscillation frequencies for 35 KEPLER solar-type planet-hosting stars using Bayesian techniques and machine learningHot super-Earths stripped by their host starsStellar spin-orbit misalignment in a multiplanet system.LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements.Radial velocity studies of cool stars.Accurate parameters for HD 209458 and its planet fromHSTspectrophotometryKepler-432 b: a massive warm Jupiter in a 52-day eccentric orbit transiting a giant starKepler-91b: a planet at the end of its lifeRadial velocity confirmation of Kepler-91 bStellar diameters and temperatures – VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfsDetection of solar-like oscillations in relics of the Milky Way: asteroseismology of K giants in M4 using data from the NASA K2 missionSpectroscopic parameters for solar-type stars with moderate-to-high rotationMagnetism, dynamo action and the solar-stellar connectionThe masses of retired A stars with asteroseismology: Kepler and K2 observations of exoplanet hostsWeighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771Testing the cores of first ascent red giant stars using the period spacing of g modesKOI-3158: The oldest known system of terrestrial-size planetsA test of the asteroseismic νmax scaling relation for solar-like oscillations in main-sequence and subgiant starsSuper-Nyquist asteroseismology of solar-like oscillators with Kepler and K2 – expanding the asteroseismic cohort at the base of the red giant branchAtmospheric parameters and chemical properties of red giants in the CoRoT asteroseismology fieldsDetecting transit signatures of exoplanetary rings using SOAP3.0Absolute masses and radii determination in multiplanetary systems without stellar modelsInferences on Stellar Activity and Stellar Cycles from AsteroseismologyAsteroseismic surface gravity for evolved starsDetecting ring systems around exoplanets using high resolution spectroscopy: the case of 51 Pegasi b
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P2860
Fundamental properties of Kepler planet-candidate host stars using asteroseismology
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im April 2013 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у квітні 2013
@uk
name
FUNDAMENTAL PROPERTIES OFKEPLERPLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
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Fundamental properties of Kepler planet-candidate host stars using asteroseismology
@en
type
label
FUNDAMENTAL PROPERTIES OFKEPLERPLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
@nl
Fundamental properties of Kepler planet-candidate host stars using asteroseismology
@en
prefLabel
FUNDAMENTAL PROPERTIES OFKEPLERPLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
@nl
Fundamental properties of Kepler planet-candidate host stars using asteroseismology
@en
P2093
P50
P356
P1476
Fundamental properties of Kepler planet-candidate host stars using asteroseismology
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P2093
Andrew W. Howard
Christopher J. Burke
Debra A. Fischer
Dennis Stello
Fergal Mullally
Hans Kjeldsen
Howard Isaacson
Jessie L. Christiansen
Michael R. Haas
Roberto Sanchis-Ojeda
P356
10.1088/0004-637X/767/2/127
P407
P50
P577
2013-04-04T00:00:00Z
P818
P819
2013ApJ...767..127H