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High energy emission from YSO jets

Christian Schneider
Hamburger Sternwarte

Abstract
Jets from young stellar objects (YSOs) are an ubiquitous phenomenon of star formation. X-ray emission from YSO jets is a recently discovered new diagnostic of the associated high-energy phenomena. About a dozen X-ray emitting jets are currently known. These detections clearly demonstrate the existence of a million degree plasma spatially close to the hundred times cooler gas usually studied. I will present recent results from high-energy observations of YSO jets and their implications for the heating, cooling and launching process.

2012 October 30, 13:30

IA/U.Porto
Centro de AstrofÝsica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto

Instituto de Astrof├şsica e Ci├¬ncias do Espa├žo Universidade do Porto Faculdade de Ciências da Universidade de Lisboa Funda├ž├úo para a Ci├¬ncia e a Tecnologia
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