activity
20242026
collaborators

5 papers

astro-ph.SR2026

Kilogauss magnetic fields from simulations of small-scale dynamo action in the convective envelope of a white dwarf

Fabio Riva, Tim Cunningham, Hans-Günter Ludwig +2

About 20% of white dwarfs are observed to host large-scale magnetic fields, but the origin of white dwarf magnetism remains uncertain. Small-scale turbulent dynamos (SSDs), which e…

astro-ph.SR2026

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis

Pierre F. L. Maxted, Nicholas Storm, Andreas J. Korn +7

AI Phe is an eclipsing binary star with an orbital period of 24.6 days for which the surface gravity and effective temperature are known from direct measurements to very high preci…

astro-ph.SR2026

Solar photospheric spectrum microvariability III. Radial velocities and line profiles in magnetic active-region granulation

Dainis Dravins, Hans-Günter Ludwig, Matthias Steffen +2

Finding low-mass planets around solar-type stars requires to understand the physical variability of the host star, which greatly exceeds the planet-induced radial-velocity modulati…

astro-ph.SR2025

Solar photospheric spectrum microvariability

Dainis Dravins, Hans-Günter Ludwig

Finding low-mass planets around solar-type stars requires to understand the physical variability of the host star, which greatly exceeds the planet-induced radial-velocity modulati…

astro-ph.SR2024

Solar photospheric spectrum microvariability II. Observed relations to magnetic activity and radial-velocity modulation

Dainis Dravins, Hans-Günter Ludwig

Searches for small exoplanets around solar-type stars are limited by stellar physical variability. While chromospheric variability is well studied, observing, modeling. and underst…