activity
20242026
collaborators

6 papers

astro-ph.SR2026

Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866

Haotian Wang, Gang Li, Dario J. Fritzewski +2

We investigate how isochrones computed with different input physics and initial conditions affect the age dating of the open cluster NGC 6866, and compare the results with asterose…

astro-ph.SR2025

Evolution of the near-core rotation frequency of 2,497 intermediate-mass stars from their dominant gravito-inertial mode

Conny Aerts, Timothy Van Reeth, Joey S. G. Mombarg +1

We combined Gaia DR3 and TESS photometric light curves to estimate the internal physical properties of 2,497 gravity-mode pulsators. We relied on asteroseismic properties of Kepler…

astro-ph.SR2024

MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators

N. Jannsen, A. Tkachenko, P. Royer +14

With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's poten…

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

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.SR2024

Estimates of (convective core) masses, radii, and relative ages for 14,000 Gaia-discovered gravity-mode pulsators monitored by TESS

Joey S. G. Mombarg, Conny Aerts, Timothy Van Reeth +1

Gravito-inertial asteroseismology saw its birth from the 4-years long light curves of rotating main-sequence stars assembled by the Kepler space telescope. High-precision measureme…