XMM-Newton observations reveal the X-ray counterpart of the very-high-energy gamma-ray source HESSJ1640-465
arXiv:astro-ph/0701166 · doi:10.1086/516567
Abstract
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.
submitted to the Astrophysical Journal
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Cited by in corpus (17)
- Teraelectronvolt Astronomy
- The soft gamma-ray pulsar population: an high-energy overview
- NuSTAR Discovery of a Young, Energetic Pulsar Associated with the Luminous Gamma-ray Source HESS J1640-465
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- Discovery of the Putative Pulsar and Wind Nebula Associated with the TeV Gamma-ray Source HESS J1813-178
- PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV Gamma-ray Source HESS J1857+026
- The GeV-TeV Connection in Galactic gamma-ray sources
- Search for Pulsar Wind Nebula Associations of Unidentified TeV Gamma-Ray Sources
- Interstellar gas towards the TeV gamma-ray sources HESS J1640-465 and HESS J1641-463
- The Norma Arm Region Chandra Survey: X-ray Populations in the Spiral Arms
- Chasing the Identification of ASCA Galactic Objects (ChIcAGO) - An X-ray Survey of Unidentified Sources in the Galactic Plane I: Source Sample and Initial Results
- HESS J1640-465 and HESS J1641-463: two intriguing TeV sources in the light of new Fermi LAT observations
- Observation of an extended VHE gamma-ray emission from MSH 15-52 with CANGAROO-III
- Constraining the origin of the puzzling source HESS J1640-465 and the PeVatron candidate HESS J1641-463 using Fermi-LAT observations
- VHE Gamma-ray supernova remnants
- Broadband X-ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465
- Using X-ray observations to identify the particle acceleration mechanisms in VHE SNRs and "dark" VHE sources