activity
20242026
collaborators

17 papers

astro-ph.SR2026

RedDots: Magnetic field of the nearby active M dwarf GJ 729, and a search for companions

E. L. Brown, S. V. Jeffers, S. C. Marsden +5

M dwarfs are prime targets for discovering exoplanets, and the nearest M dwarfs to the Sun provide among the best opportunities for follow-up detailed exoplanet characterization. G…

astro-ph.SR2026

Magnetic geometry of M dwarfs in the southern PLATO field

M. Diez, P. I. Cristofari, J. Morin +9

M dwarfs are the most abundant stars in the Galaxy and exhibit diverse magnetic behaviours. Understanding their large-scale magnetic fields is essential to study stellar dynamos an…

astro-ph.SR2026

A fast method for deriving relative small-scale magnetic field variations from high-resolution spectroscopy

Paul I. Cristofari, Steven H. Saar, Aline A. Vidotto +1

Observational constraints on stellar magnetic fields are essential to both stellar and planetary physics. Recent studies revealed the diversity and evolution of large-scale magneti…

astro-ph.SR2026

The attempted polarity reversal and evolving magnetic environment of AD Leo

K. G. Smith, D. Evensberget, S. Bellotti +3

In the past two decades, the observed large-scale magnetic field of the active M dwarf star AD Leo has evolved from strongly to mildly negative, raising a suspicion that it might s…

astro-ph.SR2025

Discovery of a rapidly evolving global magnetic field in the M-dwarf YZ Cet and constraints on the magnetic field of its planet YZ Cet b

Ayan Biswas, Colin P. Folsom, James A. Barron +3

We present a spectropolarimetric study of the nearby M4.5V exoplanet host star YZ Cet, based on near-infrared observations obtained with the SpectroPolarimètre InfraRouge (SPIRou)…

astro-ph.SR2025

Long-term X-ray variability of the multiple-planet host L 98-59: Hints of an activity cycle

I. Pillitteri, S. Bellotti, S. Benatti +7

High-energy irradiation in X-rays and UV (XUV) can transform the planetary atmospheres through photoevaporation and photochemistry. This is more crucial for M stars, whose habitabl…