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20182021
most citedA comparison of the dynamical and model-derived parameters of the pulsating eclipsing binary KIC9850387

32 citations · 57 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202132 cited

A comparison of the dynamical and model-derived parameters of the pulsating eclipsing binary KIC9850387

S. Sekaran, A. Tkachenko, C. Johnston +1

We aim to unravel the interior mixing profile of the pulsating eclipsing binary KIC9850387 by comparing its dynamical parameters and the parameters derived through a combination of…

astro-ph.SR202118 cited

Characterization of the variability in the O+B eclipsing binary HD 165246

Cole Johnston, Nicolas Aimar, Michael Abdul-Masih +8

O-stars are known to experience a wide range of variability mechanisms originating at both their surface and their near-core regions. Characterization and understanding of this var…

astro-ph.SR2020

Tango of celestial dancers: A sample of detached eclipsing binary systems containing g-mode pulsating components. A case study of KIC9850387

S. Sekaran, A. Tkachenko, M. Abdul-Masih +9

Eclipsing binary systems with components that pulsate in gravity modes ( modes) allow for simultaneous and independent constraints of the chemical mixing profiles of stars. We a…

astro-ph.SR2019

The spectroscopic binaries RV Tauri and DF Cygni

Rajeev Manick, Devika Kamath, Hans Van Winckel +7

Aim: The focus of this paper is on two famous but still poorly understood RV Tauri stars: RV Tau and DF Cyg. We aim at confirming their suspected binary nature and deriving their o…

astro-ph.SR20197 cited

Two's a crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter in red-giant binaries

Sanjay Sekaran, Cole Johnston, Andrew Tkachenko +3

Theoretical scaling relations for solar-like oscillators and red giants are widely used to estimate fundamental stellar parameters. The accuracy and precision of these relations ha…

astro-ph.SR2019

Astro2020 Science White Paper: gravity-wave asteroseismology of intermediate- and high-mass stars

Andrew Tkachenko, Conny Aerts, Dominic M. Bowman +17

The evolution of a star is driven by the physical processes in its interior making the theory of stellar structure and evolution the most crucial ingredient for not only stellar ev…