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										Seminario: Jorge Sans-Forcada (CAB, CSIC-INTA, Spain)
																			
								 
																
									Seminario: Jorge Sans-Forcada (CAB, CSIC-INTA, Spain)
																										
								
								 
									Jul 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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