Calendar
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												Meeting EXOPA
											
																							
													10:00
												
																					 
											
												Seminario: Jorge Sans-Forcada (CAB, CSIC-INTA, Spain)
											
																							
													11:30
												
																					 
																				
											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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