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HAZMAT. V. The Ultraviolet and X-ray Evolution of K Stars

By Tyler Richey-Yowell and others
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 any biosignatures could be detected, as UV radiation can severely change or destroy a planet's atmosphere. Current efforts for finding a potentially habitable... Show more
January 2, 2019
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HAZMAT. V. The Ultraviolet and X-ray Evolution of K Stars
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