activity
20182024
most citedInternal mixing of rotating stars inferred from dipole gravity modes

168 citations · 795 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2024★ 2 cited

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★ 1 cited

Photometric detection of internal gravity waves in upper main-sequence stars. IV. Comparable stochastic low-frequency variability in SMC, LMC, and Galactic massive stars

Dominic M. Bowman, Pieterjan Van Daele, Mathias Michielsen +1

Massive main-sequence stars have convective cores and radiative envelopes, but also sub-surface convection zones caused by partial ionisation. However, the convective properties de…

astro-ph.IM2024★ 2 cited

Foam: A Python package for forward asteroseismic modelling of gravity modes

Mathias Michielsen

Asteroseismology, the study of stellar pulsations, offers insights into the internal structures and evolution of stars. Analysing the variations in a star's brightness allows the d…

astro-ph.SR2024

The impact of asteroseismically calibrated internal mixing on nucleosynthetic wind yields of massive stars

Hannah E. Brinkman, Lorenzo Roberti, Alex Kemp +3

Asteroseismology gives us the opportunity to look inside stars and determine their internal properties. Based on these observations, estimations can be made for the amount of the c…

astro-ph.SR2024

The impact of radiative levitation on mode excitation of main-sequence B-type pulsators

R. Rehm, J. S. G. Mombarg, C. Aerts +3

Numerical computations of stellar oscillations for models representative of B-type stars predict fewer modes to be excited than observations reveal from modern space-based photomet…

astro-ph.SR2023

Modelling time-dependent convective penetration in 1D stellar evolution

Cole Johnston, Mathias Michielsen, Evan H. Anders +7

1D stellar evolution calculations produce uncertain predictions for quantities like the age, core mass, core compactness, and nucleo-synthetic yields; a key source of uncertainty i…