All the confirmed Soft Gamma-ray Repeaters have been observed with the EPIC instrument on the XMM-Newton satellite. We review the results obtained in these observations, providing the most accurate spectra on the persistent X-ray emission in the 1-10 keV range for these objects, and discuss them in the context of the magnetar interpretation. © Springer Science+Business Media B.V. 2007.
CITATION STYLE
Mereghetti, S., Esposito, P., & Tiengo, A. (2007). XMM-Newton observations of soft gamma-ray repeaters. In Isolated Neutron Stars: From The Surface To The Interior (pp. 13–23). Springer Netherlands. https://doi.org/10.1007/978-1-4020-5998-8_2
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