Abstract
Aims. HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously been found in longer-wavelength data, the processes that power the VHE emission are not well understood.Methods. Combining the latest VHE data with recent XMM-Newton observations and a variety of source catalogs and lower-energy survey data, we attempt to match (from an energetic and positional standpoint) the various parts of the emission of HESS J1745-303 with possible candidates.Results. Though no single counterpart is found to fully explain the VHE emission, we postulate that at least a fraction of the VHE source may be explained by a supernova-remnant/molecular-cloud association and/or a high-spin-down-flux pulsar.
Original language | English (US) |
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Pages (from-to) | 509-517 |
Number of pages | 9 |
Journal | Astronomy and Astrophysics |
Volume | 483 |
Issue number | 2 |
DOIs | |
State | Published - May 2008 |
Keywords
- Galaxy: general
- Gamma rays: observations
- ISM: clouds
- ISM: cosmic rays
- X-rays: general