Astrospheres of planet-hosting cool stars and beyond⋅ when modeling meets observations

K Herbst, LR Baalmann, A Bykov, NE Engelbrecht… - Space Science …, 2022 - Springer
Thanks to dedicated long-term missions like Voyager and GOES over the past 50 years,
much insight has been gained on the activity of our Sun, the solar wind, its interaction with …

[HTML][HTML] The solar orbiter mission-science overview

D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …

Persistence of flare-driven atmospheric chemistry on rocky habitable zone worlds

H Chen, Z Zhan, A Youngblood, ET Wolf… - Nature …, 2021 - nature.com
Low-mass stars show evidence of vigorous magnetic activity in the form of large flares and
coronal mass ejections. Such space weather events may have important ramifications for the …

Statistical properties of superflares on solar-type stars: results using all of the Kepler primary mission data

S Okamoto, Y Notsu, H Maehara… - The Astrophysical …, 2021 - iopscience.iop.org
We report the latest statistical analyses of superflares on solar-type (G-type main-sequence;
effective temperature is 5100–6000 K) stars using all of the Kepler primary mission data and …

Extreme energetic particle events by superflare-associated CMEs from solar-like stars

J Hu, VS Airapetian, G Li, G Zank, M Jin - Science Advances, 2022 - science.org
Discovery of frequent superflares on active cool stars opened a new avenue in
understanding the properties of eruptive events and their impact on exoplanetary …

Apache Point Observatory (APO)/SMARTS flare star campaign observations. I. Blue wing asymmetries in chromospheric lines during Mid-M-Dwarf flares from …

Y Notsu, AF Kowalski, H Maehara… - The Astrophysical …, 2024 - iopscience.iop.org
We conducted the time-resolved simultaneous optical spectroscopic and photometric
observations of mid-M-dwarf flare stars YZ CMi, EV Lac, and AD Leo. Spectroscopic …

Impact of stellar flares on the chemical composition and transmission spectra of gaseous exoplanets orbiting M dwarfs

T Konings, R Baeyens, L Decin - Astronomy & Astrophysics, 2022 - aanda.org
Context. Stellar flares of active M dwarfs can affect the atmospheric composition of close-
orbiting gas giants, and can result in time-dependent transmission spectra. Aims. We aim to …

A Superflare on YZ Canis Minoris Observed by the Seimei Telescope and TESS: Red Asymmetry of Hα Emission Associated with White-light Emission

K Namizaki, K Namekata, H Maehara… - The Astrophysical …, 2023 - iopscience.iop.org
Active M-type stars are known to often produce superflares on the surface. Radiation from
stellar (super) flares is important for exoplanet habitability, but the mechanisms are not well …

From starspots to stellar coronal mass ejections—revisiting empirical stellar relations

K Herbst, A Papaioannou, VS Airapetian… - The Astrophysical …, 2021 - iopscience.iop.org
Upcoming missions, including the James Webb Space Telescope, will soon characterize the
atmospheres of terrestrial-type exoplanets in habitable zones around cool K-and M-type …

Sun-as-a-star Analysis of Hα Spectra of a Solar Flare Observed by SMART/SDDI: Time Evolution of Red Asymmetry and Line Broadening

K Namekata, K Ichimoto, TT Ishii… - The Astrophysical …, 2022 - iopscience.iop.org
Stellar flares sometimes show red/blue asymmetries of the Hα line, which can indicate
chromospheric dynamics and prominence activations. However, the origin of asymmetries is …