Long-term X-ray variability of the multiple-planet host L 98-59: Hints of an activity cycle
I. Pillitteri (1), S. Bellotti (2, 3), S. Benatti (1), S. Boro Saikia (4), A. Garc\'ia Mu\~noz (5), K. G. Kislyakova (4), A. Maggio (1), G. Micela (1), K. Vida (6, 7), and A. A. Vidotto (2) ((1) INAF-Osservatorio Astronomico di Palermo, Italy (2) Leiden Observatory

TL;DR
This study monitors the X-ray activity of the M dwarf star L 98-59 over multiple years, revealing a potential 2-year activity cycle and assessing the impact of stellar X-ray radiation on its habitable-zone planets.
Contribution
First long-term X-ray monitoring of L 98-59 revealing possible activity cycles and their implications for planetary habitability.
Findings
Detected significant X-ray flares in 2020-2021.
Estimated an approximately 2-year activity cycle.
Found outer planet exposed to high X-ray doses.
Abstract
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 habitable zones for Earth-like planets are located within a few percent of an AU. Transiting exoplanets around M dwarfs offer the opportunity to study their characteristics and habitability conditions. L 98-59 is an M3 dwarf hosting six Earth-like planets, with two of them in the habitable zone of the star. X-ray observations made in 2020 and 2021 detected significant flares above a quiescent luminosity of 4-10 x 10^26 erg/s. We present the results from two short XMM-Newton observations of L 98-59, which are part of a monitoring survey to detect long-term X-ray variability and activity cycles. In October 2024 the X-ray quiescent luminosity of the star was about 5.9 x 10^25 erg/s, and it was about 6.3 x 10^26 erg/s in…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysical Phenomena and Observations
