activity
20122020
most citedTesting the asteroseismic scaling relations for Red Giants with Eclipsing Binaries Observed by Kepler

195 citations · 542 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2020★ 19 cited

Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections

J. M. Joel Ong, Sarbani Basu, Jean M. McKeever

Localised modelling error in the near-surface layers of evolutionary stellar models causes the frequencies of their normal modes of oscillation to differ from those of actual stars…

astro-ph.IM2020★ 24 cited

Fast and Automated Peak Bagging with DIAMONDS (FAMED)

E. Corsaro, J. M. McKeever, J. S. Kuszlewicz

Stars of low and intermediate mass that exhibit oscillations may show tens of detectable oscillation modes each. Oscillation modes are a powerful to constrain the internal structur…

astro-ph.SR2020★ 50 cited

Active red giants: close binaries versus single rapid rotators

Patrick Gaulme, Jason Jackiewicz, Federico Spada +7

The objective of this work is to determine what fraction of red-giant (RG) stars shows photometric rotational modulation, and understand its origin. One of the underlying questions…

astro-ph.SR2019★ 33 cited

The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations

Jean McKeever, Sarbani Basu, Enrico Corsaro

The helium abundance of stars is a strong driver of evolutionary timescales, however it is difficult to measure in cool stars. We conduct an asteroseismic analysis of NGC 6791, an…

astro-ph.SR2017★ 1 cited

Modeling Radial Velocities and Eclipse Photometry of the Kepler Target KIC 4054905: an Oscillating Red Giant in an Eclipsing Binary

M. Benbakoura, P. Gaulme, J. McKeever +3

Asteroseismology is a powerful tool to measure the fundamental properties of stars and probe their interiors. This is particularly efficient for red giants because their modes are…

astro-ph.SR2016★ 195 cited

Testing the asteroseismic scaling relations for Red Giants with Eclipsing Binaries Observed by Kepler

Patrick Gaulme, Jean McKeever, Jason Jackiewicz +7

Given the potential of ensemble asteroseismology for understanding fundamental properties of large numbers of stars, it is critical to determine the accuracy of the scaling relatio…

astro-ph.SR2016★ 49 cited

KIC 9246715: The Double Red Giant Eclipsing Binary With Odd Oscillations

Meredith L. Rawls, Patrick Gaulme, Jean McKeever +7

We combine Kepler photometry with ground-based spectra to present a comprehensive dynamical model of the double red giant eclipsing binary KIC 9246715. While the two stars are very…

astro-ph.GA2013★ 3 cited

Interstellar Absorption Lines in the Direction of the Cataclysmic Variable SS Cygni

Adam M. Ritchey, George Wallerstein, Jean McKeever

We present an analysis of interstellar absorption lines in high-resolution optical echelle spectra of SS Cyg obtained during an outburst in 2013 June and in archival Hubble Space T…

astro-ph.SR2013★ 32 cited

Two new SB2 binaries with main sequence B-type pulsators in the Kepler field

P. I. Pápics, A. Tkachenko, C. Aerts +15

Context: OB stars are important in the chemistry and evolution of the Universe, but the sample of targets well understood from an asteroseismological point of view is still too lim…

astro-ph.SR2013★ 79 cited

Red Giants in Eclipsing Binary and Multiple-Star Systems: Modeling and Asteroseismic Analysis of 70 Candidates from Kepler Data

Patrick Gaulme, Jean Mc Keever, Meredith L. Rawls +3

Red-giant stars are an incredible source of information for testing models of stellar evolution, as asteroseismology has opened up a window into their interiors. Such insights are…

astro-ph.SR2012★ 57 cited

The Classificiation of Kepler B star Variables

Bernard J. McNamara, Jason Jackiewicz, Jean McKeever

The light curves of 252 B-star candidates in the Kepler data base are analyzed in a similar fashion to that done by Balona et al. (2011) to further characterize B star variability,…