activity
20122026
most citedMagnetic moment and plasma environment of HD 209458b as determined from Ly observations

153 citations · 2.7k across the 58 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026

Star Planet Interactions

Arghyadeep Paul, Kristina Kislyakova, Manuel Güdel +13

Star-planet interactions (SPIs) describe the continuous exchange of energy, momentum, and mass between exoplanets and their host stars through radiative, tidal, magnetic, and parti…

astro-ph.SR2026

Stellar Forcing of (exo)Planetary Environments

Julián D. Alvarado-Gómez, Erika Palmerio, Manuel Güdel +13

The environments of exoplanets are fundamentally shaped by the magnetic activity of their host stars through radiative, plasma, and particle-driven processes. This article presents…

astro-ph.SR2025★ 1 cited

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…

astro-ph.SR2025

First Resolution of a Main Sequence G-Star Astrosphere Using Chandra

C. M. Lisse, S. J. Wolk, B. Snios +24

We report resolution of a halo of X-ray line emission surrounding the Zero Age Main Sequence (ZAMS) G8.5V star HD 61005 by Chandra ACIS-S. Located only 36.4 pc distant, HD 61005 is…

astro-ph.SR2024★ 14 cited

X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates

K. G. Kislyakova, M. Güdel, D. Koutroumpa +3

Stellar winds of cool main sequence stars are very difficult to constrain observationally. One way to measure stellar mass loss rates is to detect soft X-ray emission from stellar…

astro-ph.SR2023★ 4 cited

Non-thermal motions and atmospheric heating of cool stars

S. Boro Saikia, T. Lueftinger, V. S. Airapetian +6

The magnetic processes associated with the non-thermal broadening of optically thin emission lines appear to carry enough energy to heat the corona and accelerate the solar wind. W…