activity
20052021
most citedAsteroseismic masses, ages, and core properties of Doradus stars using gravito-inertial dipole modes and spectroscopy

97 citations · 182 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2021

Internal mixing of rotating stars inferred from dipole gravity modes

May G. Pedersen, Conny Aerts, Péter I. Pápics +7

During most of their life, stars fuse hydrogen into helium in their cores. The mixing of chemical elements in the radiative envelope of stars with a convective core is able to repl…

astro-ph.SR201942 cited

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

L. Decin, W. Homan, T. Danilovich +12

In 1981, the idea of a superwind that ends the life of cool giant stars was proposed. Extreme OH/IR-stars develop superwinds with the highest mass-loss rates known so far, up to a…

astro-ph.SR201997 cited

Asteroseismic masses, ages, and core properties of Doradus stars using gravito-inertial dipole modes and spectroscopy

Joey S. G. Mombarg, Timothy Van Reeth, May G. Pedersen +5

The asteroseismic modelling of period spacing patterns from gravito-inertial modes in stars with a convective core is a high-dimensional problem. We utilise the measured period spa…

astro-ph.SR2018

Binary Asteroseismic Modelling: isochrone-cloud methodology and application to Kepler gravity-mode pulsators

C. Johnston, A. Tkachenko, C. Aerts +5

The simultaneous presence of variability due to both pulsations and binarity is no rare phenomenon. Unfortunately, the complexities of dealing with even one of these sources of var…

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…

astro-ph200743 cited

The variable mass loss of the AGB star WX Psc as traced by the CO J=1-0 through 7-6 lines and the dust emission

L. Decin, S. Hony, A. de Koter +3

Low and intermediate mass stars lose a significant fraction of their mass through a dust-driven wind during the Asymptotic Giant Branch (AGB) phase. Recent studies show that winds…