Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/49608
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dc.contributor.author | Aharonian, F. | - |
dc.contributor.author | Akhperjanian, A. | - |
dc.contributor.author | Bazer-Bachi, A. | - |
dc.contributor.author | Behera, B. | - |
dc.contributor.author | Beilicke, M. | - |
dc.contributor.author | Benbow, W. | - |
dc.contributor.author | Berge, D. | - |
dc.contributor.author | Bernlohr, K. | - |
dc.contributor.author | Boisson, C. | - |
dc.contributor.author | Bolz, O. | - |
dc.contributor.author | Borrel, V. | - |
dc.contributor.author | Braun, I. | - |
dc.contributor.author | Brion, E. | - |
dc.contributor.author | Brown, A. | - |
dc.contributor.author | Buhler, R. | - |
dc.contributor.author | Busching, I. | - |
dc.contributor.author | Boutelier, T. | - |
dc.contributor.author | Carrigan, S. | - |
dc.contributor.author | Chadwick, P. | - |
dc.contributor.author | Chounet, L. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2007 | - |
dc.identifier.citation | Astronomy and Astrophysics: a European journal, 2007; 469(1):L1-L4 | - |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.issn | 1432-0746 | - |
dc.identifier.uri | http://hdl.handle.net/2440/49608 | - |
dc.description | Letter to the Editor | - |
dc.description.abstract | Aims. The complex Monoceros Loop SNR/Rosette Nebula region contains several potential sources of very-high-energy (VHE) γ-ray emission and two as yet unidentified high-energy EGRET sources. Sensitive VHE observations are required to probe acceleration processes in this region. Methods. The HESS telescope array has been used to search for very high-energy γ-ray sources in this region. CO data from the NANTEN telescope were used to map the molecular clouds in the region, which could act as target material for γ-ray production via hadronic interactions. Results. We announce the discovery of a new γ-ray source, HESS J0632+057, located close to the rim of the Monoceros SNR. This source is unresolved by HESS and has no clear counterpart at other wavelengths but is possibly associated with the weak X-ray source 1RXS J063258.3+054857, the Be-star MWC148 and/or the lower energy γ-ray source 3EGJ0634+0521. No evidence for an associated molecular cloud was found in the CO data. | - |
dc.description.statementofresponsibility | F. A. Aharonian ... G. Rowell ... et al. | - |
dc.language.iso | en | - |
dc.publisher | EDP Sciences | - |
dc.rights | © ESO 2007. Article published by EDP Sciences | - |
dc.source.uri | http://dx.doi.org/10.1051/0004-6361:20077299 | - |
dc.subject | gamma rays: observations | - |
dc.title | Discovery of a point-like very-high-energy γ-ray source in Monoceros | - |
dc.title.alternative | Discovery of a point-like very-high-energy gamma-ray source in Monoceros | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1051/0004-6361:20077299 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
Appears in Collections: | Aurora harvest Chemistry and Physics publications |
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hdl_49608.pdf | Published Version | 219.35 kB | Adobe PDF | View/Open |
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