Multiwavelength Observations of the Soft Gamma Repeater SGR 1900+14 during Its 2001 April Activation
Hurley, K.; Kouveliotou, C.; Fender, R. P.; Weisskopf, M. C.; Göǧüş, E.; Garrington, S. T.; Tennant, A.; Woods, P. M.; Patel, S. K.
United States, Netherlands, United Kingdom
Abstract
The soft gamma repeater SGR 1900+14 became active on 2001 April 18 after about 2 years of quiescence; it had remained at a very low state of activity since the fall of 1998, when it exhibited extraordinary flaring. We have observed the source in the gamma-rays and X-rays with Ulysses and Chandra and in the radio with MERLIN. We report here the confirmation of a two-component X-ray spectrum (power law + blackbody), indicating emission from the neutron star surface. We have determined that there is a dust halo, due to scattering in the interstellar medium, surrounding the source that extends up to >~100" from the center of SGR 1900+14.