{ "id": "0912.4229", "version": "v1", "published": "2009-12-21T18:39:38.000Z", "updated": "2009-12-21T18:39:38.000Z", "title": "HESS J1507-622: an unique unidentified source off the Galactic Plane", "authors": [ "O. Tibolla", "W. Domainko", "W. Hofmann", "O. de Jager", "S. Kaufmann", "N. Komin", "K. Kosack", "for the H. E. S. S. Collaboration" ], "categories": [ "astro-ph.HE" ], "abstract": "Galactic very high energy (VHE, > 100 GeV) gamma ray sources in the inner Galaxy H.E.S.S. survey tend to cluster within 1 degree in latitude around the Galactic plane. HESS J1507-622 instead is unique, since it is located at latitude of ~3.5 degrees. HESS J1507-622 is slightly extended over the PSF of the instrument and hence its Galactic origin is clear. The search for counterparts in other wavelength regimes (radio, infrared and X-rays) failed to show any plausible counterparts; and given its position off the Galactic plane and hence the absorption almost one order of magnitude lower, it is very surprising to not see any counterparts especially at X-rays wavelengths (by ROSAT, XMM Newton and Chandra). Its latitude implies that it is either rather close, within about 1 kpc, or is located well off the Galactic plane. And also the models reflect the uniqueness of this object: a leptonic PWN scenario would place this source due to its quite small extension to multi-kpc distance whereas a hadronic scenario would preferentially locate this object at distances of < 1 kpc where the density of target material is higher.", "revisions": [ { "version": "v1", "updated": "2009-12-21T18:39:38.000Z" } ], "analyses": { "keywords": [ "galactic plane", "unique unidentified source", "counterparts", "leptonic pwn scenario", "quite small extension" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 840906, "adsabs": "2009arXiv0912.4229T" } } }