A 0.8-2.4 Micron Transmission Spectrum of the Hot Jupiter CoRoT-1b
published by Everett Schlawin
in 2014
in Physics
and research's language is
English
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Abstract in English
Hot Jupiters with brightness temperatures > ~2000K can have TiO and VO molecules as gaseous species in their atmospheres. The TiO and VO molecules can potentially induce temperature