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- W124593896 abstract "I present examples of X-ray observations of young stars obtained with current X-ray observatories Chandra and XMM/Newton. The high spatial resolution of Chandra allows us to spatially resolve very crowded star forming regions (SFRs), where X-rays are able to penetrate through the circumstellar material of yet embedded, very young stars. Therefore we are able to identify new members of SFR and to study in detail X-ray properties of stars in the first phases of their life. On the other side, XMM/Newton with its large effective area, makes possible to study spectral and variability properties with a detail never" @default.
- W124593896 created "2016-06-24" @default.
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- W124593896 date "2004-01-01" @default.
- W124593896 modified "2023-09-26" @default.
- W124593896 title "X-ray observations of young stars" @default.
- W124593896 hasPublicationYear "2004" @default.
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