activity
20082026
most citedRelation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity

91 citations · 1.1k across the 52 of their papers we have counts for

collaborators

49 papers

astro-ph.SR2026

The Volans-Carina association An X-ray Bridge Between Younger and Older Stellar Populations

Daniela Muñoz-Giraldo, Beate Stelzer, Alex Binks +3

Nearby young moving groups (NYMGs) provide benchmarks for studying the evolution of magnetic activity and planetary environments at early ages. The Volans-Carina association (VCA),…

astro-ph.SR2024★ 3 cited

Long-term stellar activity of M dwarfs: A combined K2 and TESS study of two early M-type stars

St. Raetz, B. Stelzer

Studies of the rotation and activity of M type stars are essential to enhance our understanding of stellar dynamos and angular momentum evolution. Using the outstanding photometric…

astro-ph.SR2024★ 6 cited

Transitions in magnetic behavior at the substellar boundary

E. Magaudda, B. Stelzer, R. A. Osten +3

We aim at advancing our understanding of magnetic activity and the underlying dynamo mechanism at the end of the main-sequence. To this end, we collected simultaneous X-ray and rad…

astro-ph.SR2023★ 17 cited

Complete X-ray census of Mdwarfs in the solar Neighborhood I. GJ 745 AB: Coronal-hole Stars in the 10 pc Sample

M. Caramazza, B. Stelzer, E. Magaudda +4

We have embarked in a systematic study of the X-ray emission in a volume-limited sample of M dwarf stars, in order to explore the full range of activity levels present in their cor…

astro-ph.SR2022★ 24 cited

The Great Flare of 2021 November 19 on AD Leo. Simultaneous XMM-Newton and TESS observations

B. Stelzer, M. Caramazza, St. Raetz +2

We present a detailed analysis of a superflare on the active M dwarf star AD Leonis. The event presents a rare case of a stellar flare observed simultaneously in X-rays (with XMM-N…

astro-ph.SR2022★ 25 cited

Flares and rotation of M dwarfs with habitable zones accessible to TESS planet detections

B. Stelzer, M. Bogner, E. Magaudda +1

We characterize the magnetic activity of M dwarfs to provide the planet community with information on the energy input from the star; in particular, in addition to the frequency of…