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- W2100033313 abstract "Abstract We present new observations of the emission spectrum of the hot Jupiter TrES-4 designed to test the theory that the presence of temperature inversions in the atmospheres of these planets are correlated with the amount of radiation received by the planet. Our observations reveal that TrES-4 has an emission spectrum similar to that of HD 209458b, which requires the presence of an inversion layer high in the atmosphere and water emission bands in order to explain the observed features, providing additional support for that theory. We also present new observations of the thermal phase curve of HD 189733b at 24 μm, which we combine with our previous observations at 8 μm to examine how circulation in this planet's atmosphere varies as a function of depth. We discuss the relationship between the strength of the day-night circulation on both planets and their other observable properties, in particular their emission spectra." @default.
- W2100033313 created "2016-06-24" @default.
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- W2100033313 date "2008-05-01" @default.
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- W2100033313 title "Characterizing the Atmospheres of Hot Jupiters: From Spectra to Multi-Color Maps" @default.
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- W2100033313 doi "https://doi.org/10.1017/s1743921308026471" @default.
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