Search Results - "Creevey, O."
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Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology
Published in Monthly notices of the Royal Astronomical Society (11-09-2015)“…We present a study of 33 Kepler planet-candidate host stars for which asteroseismic observations have sufficiently high signal-to-noise ratio to allow…”
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A UNIFORM ASTEROSEISMIC ANALYSIS OF 22 SOLAR-TYPE STARS OBSERVED BY KEPLER
Published in The Astrophysical journal (20-04-2012)“…Asteroseismology with the Kepler space telescope is providing not only an improved characterization of exoplanets and their host stars, but also a new window…”
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Rotation periods and seismic ages of KOIs – comparison with stars without detected planets from Kepler observations
Published in Monthly notices of the Royal Astronomical Society (11-02-2016)“…One of the most difficult properties to derive for stars is their age. For cool main-sequence stars, gyrochronology relations can be used to infer stellar ages…”
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A Stellar Model-fitting Pipeline for Asteroseismic Data from the Kepler Mission
Published in The Astrophysical journal (01-07-2009)Get full text
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Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission
Published in Science (American Association for the Advancement of Science) (08-04-2011)“…In addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of…”
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PLATO as it is: A legacy mission for Galactic archaeology
Published in Astronomische Nachrichten (01-07-2017)“…Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high‐resolution chrono‐chemo‐kinematical…”
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A large sample of calibration stars for Gaia: log g from Kepler and CoRoT fields
Published in Monthly notices of the Royal Astronomical Society (21-05-2013)“…Asteroseismic data can be used to determine stellar surface gravities with precisions of <0.05 dex by using the global seismic quantities 〈Δν〉 and νmax along…”
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Asteroseismology of Solar-Type Stars with K2: Detection of Oscillations in C1 Data
Published in Publications of the Astronomical Society of the Pacific (01-10-2015)“…We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We…”
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Accurate effective temperatures of the metal-poor benchmark stars HD 140283, HD 122563, and HD 103095 from CHARA interferometry
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2018)“…Abstract Large stellar surveys of the Milky Way require validation with reference to a set of ‘benchmark’ stars whose fundamental properties are well…”
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The Complementary Roles of Interferometry and Asteroseismology in Determining the Mass of Solar-Type Stars
Published in The Astrophysical journal (10-04-2007)“…How important is an independent diameter measurement for the determination of stellar parameters of solar-type stars? When coupled with seismic observables,…”
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Constraining the Properties of Delta Scuti Stars Using Spectroscopic Eclipsing Binary Systems
Published in The Astrophysical journal (20-05-2011)“…Many stars exhibit stellar pulsations, favoring them for asteroseismic analyses. Interpreting the oscillations requires some knowledge of the oscillation mode…”
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Asteroseismology and interferometry
Published in The Astronomy and astrophysics review (01-11-2007)“…Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the…”
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A New Detached M Dwarf Eclipsing Binary
Published in The Astrophysical journal (01-06-2005)“…We describe a newly discovered detached M dwarf eclipsing binary system. This system was first observed by the TrES network during a long-term photometry…”
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CHARACTERIZING TWO SOLAR-TYPE KEPLER SUBGIANTS WITH ASTEROSEISMOLOGY: KIC 10920273 AND KIC 11395018
Published in The Astrophysical journal (20-01-2013)“…Determining fundamental properties of stars through stellar modeling has improved substantially due to recent advances in asteroseismology. Thanks to the…”
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A semi–automatic procedure for abundance determination of A– and F–type stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2009)“…A variety of physical processes leading to different types of pulsations and chemical compositions are observed between A– and F–type stars. To investigate the…”
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Testing Asteroseismic Scaling Relations with Interferometry
Published in EPJ Web of conferences (01-01-2015)“…The asteroseismic scaling relations for the frequency of maximum oscillation power, vmax, and the large frequency separation, Δν, provide an easy way to…”
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Benchmarking the effective temperature scale of red giant branch stellar models: the case of the metal-poor halo giant HD 122563
Published 05-04-2024“…A&A 689, A243 (2024) There is plenty of evidence in the literature of significant discrepancies between the observations and models of metal-poor red giant…”
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Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI
Published 21-03-2023“…A&A 674, A146 (2023) The ages of pulsating stars in clusters can be determined by isochrone fitting and it can be further improved by asteroseismic modelling…”
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Preparing the COROT Space Mission: New Variable Stars in the Galactic Anticenter Direction
Published in The Astrophysical journal (01-05-2005)Get full text
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