Young stellar objects from soft to hard X-rays

Details Young stellar objects from soft to hard X-rays Young stellar objects from soft to hard X-rays

2009-04-07

arxiv.org/abs/0904.1132v1

AIP Conf.Proc.1126:341-346,2009

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Proc. "Simbol-X: Focusing on the Hard X-Ray Universe", Paris, 2-5 Dec. 2008, ed. J. Rodriguez and P. Ferrando, in press; 6 pag

Scientific paper

10.1063/1.3149449

Magnetically active stars are the sites of efficient particle acceleration and plasma heating, processes that have been studied in detail in the solar corona. Investigation of such processes in young stellar objects is much more challenging due to various absorption processes. There is, however, evidence for violent magnetic energy release in very young stellar objects. The impact on young stellar environments (e.g., circumstellar disk heating and ionization, operation of chemical networks, photoevaporation) may be substantial. Hard X-ray devices like those carried on Simbol-X will establish a basis for detailed studies of these processes.

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