High-velocity collisions between main-sequence stars near supermassive black holes should produce bright, fast-fading ultraviolet flares whose light curves and spectra correlate with the collision parameters.
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Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
High-velocity collisions between main-sequence stars near supermassive black holes should produce bright, fast-fading ultraviolet flares whose light curves and spectra correlate with the collision parameters.