Search Results - "ELSWORTH, Y"
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Detection of solar-like oscillations in relics of the Milky Way: asteroseismology of K giants in M4 using data from the NASA K2 mission
Published in Monthly notices of the Royal Astronomical Society (01-09-2016)“…Asteroseismic constraints on K giants make it possible to infer radii, masses and ages of tens of thousands of field stars. Tests against independent estimates…”
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A Combined Analysis of the Observational Aspects of the Quasi-biennial Oscillation in Solar Magnetic Activity
Published in Space science reviews (01-12-2014)“…Solar quasi-biennial oscillations (QBOs) with the time scale of 0.6–4 yrs appear to be a basic feature of the Sun’s activity. Observational aspects of QBOs are…”
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Nitrogen depletion in field red giants: mixing during the He flash?
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…We combine simultaneous constraints on stellar evolutionary status from asteroseismology, and on nitrogen abundances derived from large spectroscopic surveys,…”
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Asteroseismology of old open clusters with Kepler: direct estimate of the integrated red giant branch mass-loss in NGC 6791 and 6819
Published in Monthly notices of the Royal Astronomical Society (01-01-2012)“…Mass-loss of red giant branch (RGB) stars is still poorly determined, despite its crucial role in the chemical enrichment of galaxies. Thanks to the recent…”
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Hot super-Earths stripped by their host stars
Published in Nature communications (11-04-2016)“…Simulations predict that hot super-Earth sized exoplanets can have their envelopes stripped by photoevaporation, which would present itself as a lack of these…”
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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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Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni
Published in Monthly notices of the Royal Astronomical Society (21-01-2015)“…The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an…”
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Mirror principle and the red-giant bump: the battle of entropy in low-mass stars
Published in Monthly notices of the Royal Astronomical Society (11-03-2020)“…ABSTRACT The evolution of low-mass stars into red giants is still poorly understood. During this evolution the core of the star contracts and, simultaneously,…”
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Low-degree solar rotational splitting from 45 yr of BiSON observations
Published in Monthly notices of the Royal Astronomical Society (21-09-2023)“…ABSTRACT We present solar low-degree rotational splitting values based on a new analysis of Sun-as-a-star observations from the Birmingham Solar Oscillations…”
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Oscillation frequencies for 35 Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning
Published in Monthly notices of the Royal Astronomical Society (21-02-2016)“…Kepler has revolutionized our understanding of both exoplanets and their host stars. Asteroseismology is a valuable tool in the characterization of stars and…”
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Unexpected solar-cycle variation of acoustic mode power in Sun-as-a-star observations
Published in Monthly notices of the Royal Astronomical Society (28-06-2022)“…ABSTRACT We examine the solar-cycle variation of the power in the low-degree helioseismic modes by looking at binned power spectra from 45 yr of observations…”
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Low-frequency, low-degree solar p-mode properties from 22 years of Birmingham Solar Oscillations Network data
Published in Monthly notices of the Royal Astronomical Society (01-04-2014)“…The solar low-degree low-frequency modes of oscillation are of particular interest as their frequencies can be measured with very high precision and hence…”
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The Octave (Birmingham–Sheffield Hallam) automated pipeline for extracting oscillation parameters of solar-like main-sequence stars
Published in Monthly notices of the Royal Astronomical Society (01-03-2010)“…The number of main-sequence stars for which we can observe solar-like oscillations is expected to increase considerably with the short-cadence high-precision…”
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Oscillating red giants in eclipsing binary systems: empirical reference value for asteroseismic scaling relation
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT The internal structures and properties of oscillating red-giant stars can be accurately inferred through their global oscillation modes…”
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Performance of the Birmingham Solar-Oscillations Network (BiSON)
Published in Solar physics (01-01-2016)“…The Birmingham Solar-Oscillations Network (BiSON) has been operating with a full complement of six stations since 1992. Over 20 years later, we look back on…”
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SEISMIC EVIDENCE FOR A RAPIDLY ROTATING CORE IN A LOWER-GIANT-BRANCH STAR OBSERVED WITH KEPLER
Published in The Astrophysical journal (01-09-2012)“…Rotation is expected to have an important influence on the structure and the evolution of stars. However, the mechanisms of angular momentum transport in stars…”
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BiSON data preparation: a correction for differential extinction and the weighted averaging of contemporaneous data
Published in Monthly notices of the Royal Astronomical Society (11-07-2014)“…The Birmingham Solar Oscillations Network (BiSON) has provided high-quality high-cadence observations from as far back in time as 1978. These data must be…”
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Super-Nyquist asteroseismology of solar-like oscillators with Kepler and K2 – expanding the asteroseismic cohort at the base of the red giant branch
Published in Monthly notices of the Royal Astronomical Society (21-11-2014)“…We consider the prospects for detecting solar-like oscillations in the ‘super-Nyquist’ regime of long-cadence (LC) Kepler photometry, i.e. above the associated…”
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Characterization of red giant stars in the public Kepler data
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…The first public release of long-cadence stellar photometric data collected by the NASA Kepler mission has now been made available. In this paper, we…”
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Why should we correct reported pulsation frequencies for stellar line-of-sight Doppler velocity shifts?
Published in Monthly notices of the Royal Astronomical Society. Letters (21-11-2014)“…In the age of Kepler and CoRoT, extended observations have provided estimates of stellar pulsation frequencies that have achieved new levels of precision,…”
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