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Two magnetars: SGR 1627–41 and 1E 1547–5408
Authors:S Mereghetti  A Tiengo  P Esposito  G Vianello  A De Luca  D Götz  G Weidenspointner  A von Kienlin  GL Israel  L Stella  N Rea  R Turolla  S Zane
Institution:1. INAF-IASF Milano, v. Bassini 15, I-20133 Milano, Italy;2. CEA Saclay, DSM/IRFU/SAp, Orme des Merisiers, F-91191 Gif sur Yvette, France;3. MPE, Giessenbachstrasse, D-85741 Garching, Germany;4. INAF – Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone, Italy;5. CSIC-IEEC, Torre C5-parell, 08193 Barcelona, Spain;6. Università di Padova, via Marzolo 8, I-35131 Padova, Italy;g MSSL, UCL, Holmbury St. Mary, Dorking Surrey RH5 6NT, United Kingdom
Abstract:We describe the results obtained with Target of Opportunity observations of the galactic sources SGR 1627–41 and 1E 1547–5408. These two transients show several similarities supporting the interpretation of Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters as a single class of strongly magnetized neutron stars.
Keywords:Neutron stars  Magnetars
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