XMM-Newton observations reveal the X-ray counterpart of the very-high-energy gamma-ray source HESSJ1640-465
- ,
- ,
- ,
- ,
8 pages
Published in:
- Astrophys.J. 662 (2007) 517-524
e-Print:
- astro-ph/0701166 [astro-ph]
DOI:
Report number:
- SLAC-PUB-12295
Citations per year
Abstract: (arXiv)
We present X-ray observations of the as of yet unidentified very high-energy (VHE) gamma-ray source HESSJ1640-465 with the aim of establishing a counterpart of this source in the keV energy range, and identifying the mechanism responsible for the VHE emission. The 21.8 ksec XMM-Newton observation of HESSJ1640-465 in September 2005 represents a significant improvement in sensitivity and angular resolution over previous ASCA studies in this region. These new data show a hard-spectrum X-ray emitting object at the centroid of the H.E.S.S. source, within the shell of the radio Supernova Remnant (SNR) G338.3-0.0. This object is consistent with the position and flux previously measured by both ASCA and Swift-XRT but is now shown to be significantly extended. We argue that this object is very likely the counterpart to HESSJ1640-465 and that both objects may represent the Pulsar Wind Nebula of an as of yet undiscovered pulsar associated with G338.3-0.0.- gamma ray: cosmic radiation
- X-ray: cosmic radiation
- cosmic radiation: particle source
- cosmic radiation: energy spectrum
- pulsar
- counters and detectors: satellite
- experimental results
References(30)
Figures(0)