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A 0.8-2.4 Micron Transmission Spectrum of the Hot Jupiter CoRoT-1b

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 نشر من قبل Everett Schlawin
 تاريخ النشر 2014
  مجال البحث فيزياء
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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



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