A. Camero-Arranz, N. Rea, M. A. McLaughlin, N. Bucciantini, P. Slane, B. Gaensler, D. Torres, L. Stella, E. de Onña, G. Israel, F. Camilo, A. Possenti
Published 2012-11-30Version 1
We present new imaging and spectral analysis of the recently discovered extended X-ray emission around the high-magnetic-field rotating radio transient RRAT J1819-1458. We used two Chandra observations, taken on 2008 May 31 and 2011 May 28. The diffuse X-ray emission was detected with a significance of ~19sigma in the image obtained by combining the two observations. Long-term spectral variability has not been observed. Possible scenarios for the origin of this diffuse X-ray emission, further detailed in Camero-Arranz et al. (2012), are here discussed.
Comments: Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 4 pages, 3 figures
Timing and Spectral Analysis of HMXB OAO 1657-415 with NuSTAR
Suzaku Observation of the Diffuse X-Ray Emission from the Open Cluster Westerlund 2: a Hypernova Remnant?
Timing and spectral analysis of the HMXB 4U 1700-37 observed with Insight-HXMT
![QR code for arXiv:1211.7350 [astro-ph.HE]](http://oss.arxitics.com/images/favicon.svg)