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Fig. 11

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Left: comparison of the atmospheric composition of GJ 436b using σCO2(300 K) (dotted line) and σCO2(550 K) (full line) when the planet orbits an M star (top), a G star (middle) and an F star (bottom). Right: differences in abundances (in %) between the results obtained with σCO2(300 K) and σCO2(550 K) for species that have an abundance superior to 10-10, for an M star (top), a G star (middle), and an F star (bottom).

This figure is made of several images, please see below:
thumbnail Open with DEXTER Download original image
thumbnail Open with DEXTER Download original image

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