Doppler shifts and spectral line profile changes in the starlight scattered from an exoplanet
Monthly Notices of the Royal Astronomical Society(2020)
Abstract
Scattered starlight from an exoplanet, commonly called reflected light, can be used to characterize the planet including the determination of its albedo and inclination of orbit. The relatively low flux ratio between directly observed starlight and starlight scattered off hot Jupiters make these systems the prime candidates for detection of reflected light using high-resolution spectroscopy. The f...
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Key words
techniques: spectroscopic,planet–star interactions,stars: rotation
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