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Seminario: Jorge Sans-Forcada (CAB, CSIC-INTA, Spain) 11:30
Seminario: Jorge Sans-Forcada (CAB, CSIC-INTA, Spain)
Lug 11@11:30–13:00
Titolo X-exoplanets and the quest for the He I 10830 triplet in exoplanets Abstract Exoplanet atmospheres photoevaporate because of XUV stellar irradiation. Evaporation signs are mainly detected through the h Lyman-alpha line, or more recently in the He I 10830 triplet. Despite of early efforts back in 2000, it was not until 2018 that the line was detected in exoplanet atmospheres.
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