Adelaide Research & Scholarship
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https://hdl.handle.net/2440/59003
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| Type: | Conference paper |
| Title: | A closer look at the unidentified TeV source HESS J1614-518 |
| Author: | Rowell, G. Horns, D. Fukui, Y. Moriguchi, Y. |
| Citation: | AIP Conference Proceedings, 2009;. pp.241-244 |
| Publisher: | Springer New York LLC |
| Publisher Place: | United States |
| Issue Date: | 2009 |
| Series/Report no.: | AIP conference Proceedings; 1085 |
| ISBN: | 9780735406162 |
| ISSN: | 0094-243X 1551-7616 |
| Conference Name: | International Meeting on High Energy Gamma-Ray Astronomy (4th : 2008 : Germany) |
| Editor: | Aharonian, F.A. Hofmann, W. Rieger, F.M. |
| Statement of Responsibility: | G. Rowell, D. Horns, (on behalf of the H.E.S.S collaboration), Y. Fukui and Y. Moriguchi |
| Abstract: | HESSJ1614-518, discovered in the H.E.S.S. Galactic Plane Survey [1], is one of the brightest unidentified or 'dark' TeV sources. No sufficiently energetic pulsars nor supernova remnants are found nearby. We review a range of recent multiwavelength data covering this source, including radio lines (NANTEN 12CO), IR (MSX), nearlR (2MASS), and X- ray energies (Swift, Suzaku, XMM). These MWL data and our comparisons with the morphology, spectra, and energetics of HESSJ1614-518 (using H.E.S.S. data up to 2007) suggest potential X-ray counterparts and a possbile connection to the highly reddended open cluster Pismis 22 (C1609-517). © 2009 American Institute of Physics. |
| Keywords: | pulsars supernova remnants gamma-rays |
| Rights: | ©2009 American Institute of Physics |
| DOI: | 10.1063/1.3076650 |
| Published version: | http://dx.doi.org/10.1063/1.3076650 |
| Appears in Collections: | Aurora harvest 5 Physics publications |
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