activity
20242026
collaborators

5 papers

astro-ph.SR2026

Sub-second cadence structure of optical flares on AD Leo

B. Schmercz, B. Seli, K. Vida +4

Stellar flares are sudden brightenings caused by magnetic reconnection and are frequently observed on late-type stars. High-cadence photometry of flares provides valuable insights…

astro-ph.SR2025

Magnetic activity on the young Sun: a case study of EK Draconis

A. Görgei, L. Kriskovics, K. Vida +8

Context. Young, solar analogue stars provide key insights into the early stages of stellar evolution, particularly in terms of magnetic activity and rotation. Their rapid rotation,…

astro-ph.SR2025

Four decades of photometry of XX Trianguli, `the most spotted star' in the sky

Zs. Kővári, K. G. Strassmeier, K. Oláh +3

Over the past 40 years the brightness variations of XX Tri, a single line RS CVn type binary system with a synchronized K-giant primary, has exceeded one magnitude in the V band. A…

astro-ph.SR2025

Starspots on eclipsing giant stars I.: The sample and eclipse mapping examples

K. Oláh, B. Seli, A. Haris +12

Spotted stars in eclipsing binary systems allow us to gather significant information about the stellar surface inhomogeneities that is otherwise impossible from only photometric da…

astro-ph.SR2024

Stellar flare morphology with TESS across the main sequence

Bálint Seli, Krisztián Vida, Katalin Oláh +5

Stellar flares are abundant in space photometric light curves. As they are now available in large enough numbers, the statistical study of their overall temporal morphology is time…