Interaction of the WAT Source in A3395 with the Intracluster Medium |
| |
| Authors: | Kiran Lakhchaura K P Singh D J Saikia R W Hunstead |
| |
| Institution: | 1.Tata Institute of Fundamental Research,Mumbai,India;2.National Centre for Radio Astrophysics,Pune,India;3.Sydney Institute for Astronomy, School of Physics,University of Sydney,NSW 2006,Australia |
| |
| Abstract: | Using X-ray observations from Chandra and XMM-Newton and radio observations from the Australia Telescope Compact Array (ATCA),
we have examined the merging environment of the bimodal cluster Abell 3395. From X-ray data we have produced thermodynamic
maps of the cluster. The Wide Angle Tail (WAT) galaxy seen in the radio is slightly offset from the X-ray emission peak of
the southern part of the cluster. The unsharp masked Chandra image of the cluster does not show any deficit in the X-ray flux
near the location of the source possibly because the thermal plasma has leaked into the cavities. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
