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HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear
Tyler Richey-Yowell, Evgenya L. Shkolnik, R. O. Parke Loyd +7
Efforts to discover and characterize habitable zone planets have primarily focused on Sun-like stars and M dwarfs. K stars, however, provide an appealing compromise between these t…
HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars
R. O. Parke Loyd, Evgenya L. Shkolnik, Adam C. Schneider +6
The ultraviolet (UV) emission from the most numerous stars in the universe, M dwarfs, impacts the formation, chemistry, atmospheric stability, and surface habitability of their pla…
HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Star
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik +4
Quantifying the evolution of stellar extreme ultraviolet (EUV, 100 -- 1000 ) emission is critical for assessing the evolution of planetary atmospheres and the h…
HAZMAT. V. The Ultraviolet and X-ray Evolution of K Stars
Tyler Richey-Yowell, Evgenya L. Shkolnik, Adam C. Schneider +3
Knowing the high-energy radiation environment of a star over a planet's formation and evolutionary period is critical in determining if that planet is potentially habitable and if…