activity
20182020
most citedLow-frequency gravity waves in blue supergiants revealed by high-precision space photometry

165 citations · 275 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020110 cited

Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy

S. Burssens, S. Simón-Díaz, D. M. Bowman +6

Lack of high-precision long-term continuous photometric data for large samples of stars has prevented the large-scale exploration of pulsational variability in the OB star regime.…

astro-ph.SR2020

The mass discrepancy in intermediate- and high-mass eclipsing binaries: the need for higher convective core masses

A. Tkachenko, K. Pavlovski, C. Johnston +6

(Abridged) Eclipsing, spectroscopic double-lined binary star systems (SB2) are excellent laboratories for calibrating theories of stellar interior structure and evolution. We aim t…

astro-ph.SR2019

Probing the shape of the mixing profile and of the thermal structure at the convective core boundary through asteroseismology

Mathias Michielsen, May G. Pedersen, Kyle C. Augustson +2

Aims: We investigate from a theoretical perspective if space asteroseismology can be used to distinguish between different thermal structures and shapes of the near-core mixing pro…

astro-ph.SR2019165 cited

Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry

Dominic M. Bowman, Siemen Burssens, May G. Pedersen +14

Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galacti…

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…

astro-ph.SR2018

Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection

C. Aerts, G. Molenberghs, M. Michielsen +13

We propose a methodological framework to perform forward asteroseismic modeling of stars with a convective core, based on gravity-mode oscillations. These probe the near-core regio…