HESS J1640-465 and HESS J1641-463: two intriguing TeV sources in the light of new Fermi LAT observations
arXiv:1409.4994 · doi:10.1088/2041-8205/794/1/L16
Abstract
We report on gamma-ray analysis of the region containing the bright TeV source HESS J1640-465 and the close-by TeV source HESS J1641-463 using 64 months of observations with the Fermi Large Area Telescope (LAT). Previously only one GeV source was reported in this region and was associated with HESS J1640-465. With an increased dataset and the improved sensitivity afforded by the reprocessed data (P7REP) of the LAT, we now report the detection, morphological study and spectral analysis of two distinct sources above 100 MeV. The softest emission in this region comes from the TeV source HESS J1641-463 which is well fitted with a power law of index Gamma = 2.47 +/- 0.05 +/- 0.06 and presents no significant gamma-ray signal above 10 GeV, which contrasts with its hard spectrum at TeV energies. The Fermi-LAT spectrum of the second TeV source, HESS J1640-465 is well described by a power-law shape of index Gamma = 1.99 +/- 0.04 +/- 0.07 that links up naturally with the spectral data points obtained by the High Energy Stereoscopic System (H.E.S.S.). These new results provide new constraints concerning the identification of these two puzzling gamma-ray sources.
Accepted for publication in ApJ Letters; 5 pages, 3 figures
References in corpus (4)
- The distance and neutral environment of the massive stellar cluster Westerlund 1
- NuSTAR Discovery of a Young, Energetic Pulsar Associated with the Luminous Gamma-ray Source HESS J1640-465
- XMM-Newton observations reveal the X-ray counterpart of the very-high-energy gamma-ray source HESSJ1640-465
- Discovery of the hard spectrum VHE gamma-ray source HESS J1641-463
Cited by in corpus (5)
- The soft gamma-ray pulsar population: an high-energy overview
- Interstellar gas towards the TeV gamma-ray sources HESS J1640-465 and HESS J1641-463
- Dense molecular gas at 12 mm towards Galactic TeV gamma-ray sources
- LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV
- Constraining the origin of the puzzling source HESS J1640-465 and the PeVatron candidate HESS J1641-463 using Fermi-LAT observations