Search Results - "Elsworth, Yvonne"
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1
Testing asteroseismology with Gaia DR2: hierarchical models of the Red Clump
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)Get full text
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Update on the APOKASC analysis of Red Giants
Published in EPJ Web of Conferences (01-01-2017)“…APOKASC is a collaboration between APOGEE's spectroscopic survey in the near IR at Apache Point (SDSS) and Kepler Asteroseismic Science Consortium (KASC) for…”
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Journal Article Conference Proceeding -
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Kepler Asteroseismology Program: Introduction and First Results
Published in Publications of the Astronomical Society of the Pacific (01-02-2010)“…Asteroseismology involves probing the interiors of stars and quantifying their global properties, such as radius and age, through observations of normal modes…”
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Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes
Published in Nature (London) (05-01-2012)“…The core values of red giant stars The core rotation rate of a star, a key indicator of its evolutionary state, cannot be measured directly because the core is…”
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Journal Article Web Resource -
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Fresh Insights on the Structure of the Solar Core
Published in The Astrophysical journal (10-07-2009)Get full text
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The APO-K2 Catalog. I. ∼7500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology
Published in The Astronomical journal (01-02-2024)“…Abstract We present a catalog of fundamental stellar properties for ∼7500 evolved stars, including stellar radii and masses, determined from the combination of…”
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Determining stellar macroturbulence using asteroseismic rotational velocities from Kepler
Published in Monthly notices of the Royal Astronomical Society (11-11-2014)Get full text
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Nature versus nurture: distinguishing effects from stellar processing and chemical evolution on carbon and nitrogen in red giant stars
Published in Monthly notices of the Royal Astronomical Society (05-04-2024)“…ABSTRACT The surface [C/N] ratios of evolved giants are strongly affected by the first dredge-up (FDU) of nuclear-processed material from stellar cores. C and…”
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ASTEROSEISMOLOGY OF THE OPEN CLUSTERS NGC 6791, NGC 6811, AND NGC 6819 FROM 19 MONTHS OF KEPLER PHOTOMETRY
Published in The Astrophysical journal (01-10-2012)“…We studied solar-like oscillations in 115 red giants in the three open clusters, NGC 6791, NGC 6811, and NGC 6819, based on photometric data covering more than…”
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Evidence for compact binary systems around Kepler red giants
Published in Monthly notices of the Royal Astronomical Society (01-08-2017)“…Abstract We present an analysis of 168 oscillating red giants from NASA's Kepler mission that exhibit anomalous peaks in their Fourier amplitude spectra. These…”
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Lifetimes and rotation within the solar mean magnetic field
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT We have used very high-cadence (sub-minute) observations of the solar mean magnetic field (SMMF) from the Birmingham Solar Oscillations Network…”
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The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way
Published in The Astronomical journal (01-05-2024)“…Abstract We present stellar age determinations for 4661 red giant branch stars in the APO-K2 catalog, derived using mass estimates from K2 asteroseismology…”
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An Asteroseismic Membership Study of the Red Giants in Three Open Clusters Observed by Kepler: NGC 6791, NGC 6819, and NGC 6811
Published in The Astrophysical journal (20-09-2011)“…Studying star clusters offers significant advances in stellar astrophysics due to the combined power of having many stars with essentially the same distance,…”
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Spatial incoherence of solar granulation: a global analysis using BiSON 2B data
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract A poor understanding of the impact of convective turbulence in the outer layers of the Sun and Sun-like stars challenges the advance towards an…”
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Evolutionary states of red-giant stars from grid-based modelling
Published in EPJ Web of Conferences (01-01-2017)“…From its surface properties it can be difficult to determine whether a red-giant star is in its heliumcore-burning phase or only burning hydrogen in a shell…”
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Journal Article Conference Proceeding -
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Stellar Spin-Orbit Misalignment in a Multiplanet System
Published in Science (American Association for the Advancement of Science) (18-10-2013)“…Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities…”
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Presence of mixed modes in red giants in binary systems
Published in EPJ Web of Conferences (01-01-2017)“…The frequencies of oscillation modes in stars contain valueable information about the stellar properties. In red giants the frequency spectrum also contains…”
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Journal Article Conference Proceeding -
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A new method for the asteroseismic determination of the evolutionary state of red-giant stars
Published in Monthly notices of the Royal Astronomical Society (21-04-2017)“…Abstract Determining the ages of red-giant stars is a key problem in stellar astrophysics. One of the difficulties in this determination is to know the…”
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Determination of Stellar Radii from Asteroseismic Data
Published in The Astrophysical journal (20-02-2010)“…The NASA Kepler mission is designed to find planets through transits. Accurate and precise radii of the detected planets depend on knowing the radius of the…”
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An In-depth Study of Grid-based Asteroseismic Analysis
Published in The Astrophysical journal (01-04-2011)“…NASA's Kepler mission is providing basic asteroseismic data for hundreds of stars. One of the more common ways of determining stellar characteristics from…”
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