activity
20242026
collaborators

9 papers

astro-ph.SR2026

Asteroseismic forward modelling of 36 Cep pulsators and inferences on their internal differential rotation

Mathijs Vanrespaille, Dario J. Fritzewski, Vincent Vanlaer +1

Asteroseismic observations of the interior rotation of main sequence stars have shown that angular momentum transport is much more efficient than expected. Which transport mechanis…

astro-ph.SR2026

Can Asteroseismic Structure Inversions Be Performed in Structure-Dependent Coordinates?

J. M. Joel Ong, Sarbani Basu, Willem Hoogendam +1

Yes. Unlike other applications of observational asteroseismology, "structure inversions" constrain the physical properties of stellar interiors in a model-independent fashion. Howe…

astro-ph.SR2026

Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue

Mykyta Kliapets, Pablo Huijse, Jeroen Audenaert +28

The PLAnetary Transits and Oscillations of stars (PLATO) mission is expected to launch in January 2027. A total of 8\% of its data rate will be dedicated to complementary science t…

astro-ph.IM2025

Expanding stellar horizons with polarized light

J. Vandersnickt, R. Ochoa Armenta, V. Vanlaer +16

The polarization of light is a critically under-utilized, rich source of information in astronomy. For stars in particular, surface magnetism polarization that can be detected and…

astro-ph.SR2025

Asteroseismic detection of an internal magnetic field in the B0.5V pulsator HD 192575

Jelle Vandersnickt, Vincent Vanlaer, Mathijs Vanrespaille +1

Internal magnetic fields are an elusive component of stellar structure. However, they can play an important role in stellar structure and evolution models through efficient angular…

astro-ph.SR2025

Is a 1D perturbative method sufficient for asteroseismic modelling of Cephei pulsators? Implications for measurements of rotation and internal magnetic fields

J. S. G. Mombarg, V. Vanlaer, S. B. Das +6

Asymmetries in the observed rotational splittings of a multiplet contain information about the star's rotation profile and internal magnetic field. However, to exploit this informa…