activity
20202026
most citedThe SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere

371 citations · 592 across the 17 of their papers we have counts for

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12 papers · 1 filter

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.SR2026

Eating planets makes you younger: The magnetic dynamo rejuvenation of GJ 504 by planetary engulfment

S. Bellotti, C. Pezzotti, G. Buldgen +3

With the discovery of a few thousand exoplanets, questions have been raised regarding star-planet interactions and whether the presence of a companion may affect stellar properties…

astro-ph.SR2025

The X-ray luminosity function of stars observed with SRG/eROSITA

Nicola Locatelli, Gabriele Ponti, Enza Magaudda +1

Background diffuse X-ray emission is contributed in large part by the emission of point sources not individually resolved. While this is established since decades for the contribut…

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.SR2024★ 7 cited

Simultaneous X-ray and optical variability of M dwarfs observed with eROSITA and TESS

W. M. Joseph, B. Stelzer, E. Magaudda +1

We study variability through simultaneous optical and X-ray observations for the first time in a statistical sample of 256 M dwarfs. Such observations are required to constrain the…

astro-ph.SR2024★ 6 cited

The high-energy environment of the heavy sub-Earth GJ 367 b indicates likely complete evaporation of its atmosphere

K. Poppenhaeger, L. Ketzer, N. Ilic +5

The planet GJ 367 b is a recently discovered high-density sub-Earth orbiting an M dwarf star. Its composition was modelled to be predominantly iron with a potential remainder of a…

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★ 6 cited

First eROSITA-TESS results for M dwarfs: Mass dependence of the X-ray activity rotation relation and an assessment of sensitivity limits

E. Magaudda, B. Stelzer, St. Raetz

We present a study of the activity-rotation relation for M dwarf stars, using new X-ray data from the ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Russian…

astro-ph.SR2021★ 50 cited

First eROSITA study of nearby M dwarfs and the rotation-activity relation in combination with TESS

E. Magaudda, Stelzer B., St. Raetz +1

We present the first study of nearby M dwarfs with the ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Russian Spektrum-Roentgen-Gamma mission (SRG). To this…

astro-ph.SR2021★ 10 cited

A first eROSITA view of ultracool dwarfs

B. Stelzer, A. Klutsch, M. Coffaro +2

We present the first X-ray detections of ultracool dwarfs (UCDs) from the first all-sky survey of the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) onboard the…

astro-ph.SR2021★ 10 cited

The aftermath of nova Cen 2013 (V1369 Cen)

Elena Mason, Steven N. Shore, Jeremy Drake +3

Context: Classical nova progenitors are cataclysmic variables and very old novae are observed to match high mass transfer rate and (relatively) long orbital period systems. However…

astro-ph.SR2020★ 91 cited

Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity

E. Magaudda, B. Stelzer, K. R. Covey +3

We present a sample of 14 M dwarf stars observed with XMM-Newton and Chandra, for which we also computed rotational periods from Kepler Two-Wheel (K2) Mission light curves. We comp…