2006/08/17 by S. Mereghetti, P. Esposito, A. Tiengo
Physics and Astronomy · #Aerospace engineering #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Conjunction (astronomy) #Context (archaeology) #Cosmology #EPIC #Gamma ray #Gamma-ray bursts and supernovae #History #Interpretation (philosophy) #Literature #Magnetar #Neutron star #Physics #Pulsars and Gravitational Waves Research #Range (aeronautics) #Satellite #Spectral line #astro-ph
paper · pdf · doi:10.1007/s10509-007-9384-0
published as Astrophys.SpaceSci.308:13-23,2007 · 10 pages, 7 figures, 3 tables - Presented at the conference "Isolated Neutron Stars: from the Surface to the Interior", London, UK, 24-28 April 2006
arxiv created 2006/08/17 · openalex publication_date 2007/03/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.