collaborators

5 papers

astro-ph.SR2026

Results from the first spectropolarimetric survey of Dor pulsators

J. Labadie-Bartz, R. Ouazzani, C. Neiner +8

Context. Magnetic fields can have an important influence on stellar structure and evolution. In intermediate-mass (A- and F-type) stars, there are many known stars with directly me…

astro-ph.SR2026

The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy

M. N. Lund, F. Grundahl, M. S. Fredslund +35

The Stellar Observations Network Group (SONG) network has operated for more than a decade, providing long-baseline, high-cadence spectroscopic observations of bright stars and the…

astro-ph.SR2026

Wildly Oscillating Stars -- Unexplained dense ridge-like frequency agglomerations in A and F type pulsators

V. Antoci, J. Labadie-Bartz, M. Swiech +14

We investigate the origin of the dense, ridge-like frequency clusters observed in a subset of A and F type pulsating stars, which we refer to as `wildly oscillating' stars (WOS). T…

astro-ph.SR2026

Near-core magnetic field strengths inferred from gravity modes in intermediate-mass stars

Oliver Durfeldt-Pedros, Victoria Antoci, Daniel Lecoanet +2

In this work, we derive upper limits for the strength of the near-core magnetic field in intermediate-mass stars, since high-order g-modes can be fully suppressed by a critical mag…

astro-ph.SR2026

Rapidly oscillating Ap stars observed with TESS. The LAMOST Ap sample and 49 Cam

Inês Rolo, Daniel L. Holdsworth, Margarida S. Cunha +4

The rapidly oscillating chemically peculiar A-type (roAp) stars offer valuable insights into the internal physical processes of all stars, but their study is challenged by their ra…