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20242026
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astro-ph.SR2026

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry

K. Thomson-Paressant, D. M. Bowman, F. Nardini +16

A wide range of variability mechanisms exist among intermediate mass and massive stars, which are not yet fully understood. Using complementary data sources for a large population…

astro-ph.SR2026

The PLATO Science Calibration and Validation Plan: Targets for the First Long-pointing Field

Konstanze Zwintz, Conny Aerts, Andrew Tkachenko +56

In order to meet the science goals of the PLATO space mission, an extensive science calibration and validation plan has been designed. This paper describes this plan, as well as th…

astro-ph.SR2025

Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars

Hannah E. Brinkman, Andrew Tkachenko, Conny Aerts

Observations of double-lined spectroscopic eclipsing binaries are ideal to study stellar evolution. They have tight model-independent constraints on their masses and radii. With th…

astro-ph.SR2025

Orbital and Physical Properties of the Pleiades Binary 27 Tau (Atlas)

G. Torres, A. Tkachenko, K. Pavlovski +12

We report new spectroscopic and interferometric observations of the Pleiades binary star Atlas, which played an important role nearly three decades ago in settling the debate over…

astro-ph.SR2024

KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern

Alex Kemp, Dario J Fritzewski, Timothy Van Reeth +7

In this work, we aim to estimate the stellar parameters of the primary (Aa) by performing asteroseismic analysis on its period-spacing pattern. We use the C-3PO neural network to p…

astro-ph.SR2024

The ESO UVES/FEROS Large Programs of TESS OB pulsators. II. On the physical origin of macroturbulence

Nadya Serebriakova, Andrew Tkachenko, Conny Aerts

Spectral lines of hot massive stars are known to exhibit large excess broadening in addition to rotational broadening. This excess broadening is often attributed to macroturbulence…