Journal of astrophysics and astronomy | |
Interaction of the WAT Source in A3395 with the Intracluster Medium | |
D. J. Saikia3  R. W. Hunstead2  Kiran Lakhchaura11  K. P. Singh1  | |
[1] Tata Institute of Fundamental Research, Mumbai 400 005, India.$$;Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia.$$;National Centre for Radio Astrophysics, Pune 411 007, India.$$ | |
关键词: Galaxies: clusters: general; galaxies: clusters: individual: (A3395); galaxies: clusters: intracluster medium; X-rays: galaxies: clusters; radio continuum: galaxies.; | |
DOI : | |
学科分类:天文学(综合) | |
来源: Indian Academy of Sciences | |
【 摘 要 】
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.
【 授权许可】
Unknown
【 预 览 】
Files | Size | Format | View |
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RO201912040493655ZK.pdf | 171KB | download |