![]() |
Figure 1: IBIS/ISGRI image of the SGR 1900+14 field in the 18-60 keV energy range. The other detected sources are the high-mass X-ray binary (HMXB) IGR J19140+0951 (Rodriguez et al. 2005), the black hole candidate XTE J1908+094 (in't Zand et al. 2002), the HMXB pulsar H 1907+097 (Makishima et al. 1984), and the weak unidentified source AXJ 1910.7+917 (Sugizaki et al. 2001). |
Open with DEXTER |
![]() |
Figure 2: Broad band X-ray spectra of the five magnetars detected by INTEGRAL. The data points above 18 keV are the INTEGRAL spectra with their best fit power-law models (dotted lines). The solid lines below 10 keV represent the absorbed power-law (dotted lines) plus blackbody (dashed lines) models taken from Woods et al. (2001) (SGR 1900+14, during a quiescent state in spring 2000), Mereghetti et al. (2005c) (SGR 1806-20, observation B, when the bursting activity was low), Göhler et al. (2005) (4U 0142+614), Rea et al. (2005) (1RXS J170849-4009), and Morii et al. (2003) (1E 1841-045). |
Open with DEXTER |