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
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Flare-driven habitability: Expanding life's potential around low-mass stars. [PDF]
Gao DY, Liu HG, Yang M, Zhou JL.
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Chromospheric lines in red dwarf flare stars. I - AD Leonis and GX Andromedae
B. R. Pettersen, L. A. Coleman
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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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Radio detection of late-type (G-K) dwarf stars in the Pleiades
We report deep 3.6 cm radio observations of a small sample of the most rapidly rotating G-K dwarf stars in the Pleiades. Of the four ultrafast rotators (UFRs) observed, three were detected.
White, SM, Lim, J
core
False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Oates S.
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