XMM-Newton observations of Soft Gamma-ray Repeaters

Details XMM-Newton observations of Soft Gamma-ray Repeaters XMM-Newton observations of Soft Gamma-ray Repeaters

2006-08-17

arxiv.org/abs/astro-ph/0608364v1

Astrophys.SpaceSci.308:13-23,2007

Astronomy and Astrophysics

Astrophysics

10 pages, 7 figures, 3 tables - Presented at the conference "Isolated Neutron Stars: from the Surface to the Interior", London

Scientific paper

10.1007/s10509-007-9384-0

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.

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