Red Stars, Green Planets: Evaluating Planetary Habitability in Light of M-Dwarf Superflares
M-dwarf stars frequently emit high-energy flares; superflares, with energies of at least $10^{33}$ erg, are not uncommon. Repeated superflares can render planets uninhabitable, but at the same time, M-dwarfs do not emit the ultraviolet radiation that ...
Glazier, Amy
core +1 more source
A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations. [PDF]
Wang J +14 more
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Starspots as the origin of ultrafast drifting radio bursts from an active M dwarf. [PDF]
Zhang J +18 more
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NuSTAR Observation of Energy Release in 11 Solar Microflares. [PDF]
Duncan J +8 more
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Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
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False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Oates S.
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Timescales for Prebiotic Photochemistry Under Realistic Surface Ultraviolet Conditions. [PDF]
Rimmer PB +7 more
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Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
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Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]
Tamburri C +9 more
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