activity
20072026
most citedThe Gaia-ESO Survey: Kinematic structure in the Gamma Velorum Cluster

133 citations · 546 across the 19 of their papers we have counts for

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10 papers · 1 filter

astro-ph.SR2026

The X-ray catalogue of FGK stars within 10 pc: The coronal temperature-brightness relation explained with the RTV scaling law

M. M. Bennedik, B. Stelzer, M. Caramazza +3

A comprehensive measurement of stellar X-ray emission has important implications for our understanding of stellar dynamos, exoplanet atmosphere loss, and evaporation of protoplanet…

astro-ph.SR2026

Quiet, but not silent. The X-ray activity of the Maunder minimum star HD 166620

M. M. Bennedik, B. Stelzer, H. Isaacson +3

As the only known unambiguous star in a Maunder minimum-like chromospheric activity state, the properties of HD 166620 can provide valuable insight into the behaviour of the Sun du…

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.SR2021★ 43 cited

The Gaia-ESO Survey: Target selection of open cluster stars

A. Bragaglia, E. Alfaro, E. Flaccomio +36

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The diffe…

astro-ph.SR2016★ 47 cited

Supersaturation and activity-rotation relation in PMS stars: the young Cluster h Per

C. Argiroffi, M. Caramazza, G. Micela +4

The magnetic activity of late-type MS stars is characterized by different regimes, and their activity levels are well described by Ro, the ratio between P_rot and the convective tu…