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20212024
most citedAngular momentum transport by magnetic fields in main sequence stars with Gamma Doradus pulsators

26 citations · 50 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

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.SR2024

Age uncertainties of red giants due to cumulative rotational mixing of progenitors calibrated by asteroseismology

D. J. Fritzewski, C. Aerts, J. S. G. Mombarg +2

Galactic archaeology largely relies on precise ages of distant evolved stars in the Milky Way. Nowadays, asteroseismology can deliver ages for many red giants observed with high-ca…

astro-ph.SR2024

A two-dimensional perspective of the rotational evolution of rapidly rotating intermediate-mass stars

Joey S. G. Mombarg, Michel Rieutord, Francisco Espinosa Lara

Recently, the first successful attempt at computing stellar models in two dimensions has been presented with models that include the centrifugal deformation and self-consistently c…

astro-ph.SR2023★ 26 cited

Angular momentum transport by magnetic fields in main sequence stars with Gamma Doradus pulsators

F. D. Moyano, P. Eggenberger, S. J. A. J. Salmon +2

Context. Asteroseismic studies showed that cores of post main-sequence stars rotate slower than theoretically predicted by stellar models with purely hydrodynamical transport proce…

astro-ph.SR2021★ 11 cited

Dynamical parallax, physical parameters and evolutionary status of the components of the bright eclipsing binary α Draconis

K. Pavlovski, C. A. Hummel, A. Tkachenko +13

Altough both components of the bright eclipsing binary Dra having been resolved using long baseline interferometry and the secondary component shown to contribute some 15\% of…