| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1767439 | Advances in Space Research | 2008 | 5 Pages |
Abstract
IC433 is a supernova remnant (SNR) interacting with a molecular cloud. The field of IC443 also contains an unidentified gamma-ray source 3EG J0617 + 2238. Recent observations with XMM-Newton and Chandra have revealed a number of hard X-ray sources in the field of the extended SNR including a pulsar wind nebula and an enigmatic hard X-ray source in the SNR – molecular cloud interaction region. We present preliminary results from INTEGRAL observations of IC443. Several sources have been detected by JEM-X, both in the 3–10 and 10–35 keV band, among which is the PWN. We discuss the relation between the JEM-X sources and the detected XMM/Chandra X-ray sources.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
F. Bocchino, A.M. Krassilchtchikov, P. Kretschmar, A.M. Bykov, Yu.A. Uvarov, S.M. Osipov,