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| HAL : in2p3-00368763, version 1 |
| Code Bibliographique ADS : 2008AIPC.1085..234G |
| DOI : 10.1063/1.3076648 |
| Fiche détaillée |  Récupérer au format |
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| 4th International Meeting on High Energy Gamma-Ray Astronomy, Heidelberg : Allemagne (2008) |
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| GMRT radio observations of HESS J1640-465 |
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| E. GiacaniG. CastellettiG. DubneB.C. JoshiP. RaoR. Terrier1 |
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| (12/2008) |
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| New high resolution and high sensitivity radio observations were conducted with the Giant Metrewave Radio Telescope (GMRT) in the direction of the γ-ray source HESS J1640-465, in positional coincidence with the supernova remnant (SNR) G338.3-0.0. The new images, obtained at 235 MHz and at 610 MHz, allow us to confirm that G338.3-0.0 is a typical shell-like remnant. No sign of the existence of a pulsar wind nebula or a radio pulsar is detected in its interior. Whether the high-energy particles are accelerated at the SNR shell or associated with an undetected pulsar, is still an open question. |
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| 1 : | APC - AstroParticule et Cosmologie |
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| APC - AHE |
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| Thème(s) | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie |
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| supernova remnants – radioactive sources – pulsars |
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| in2p3-00368763, version 1 | |
| http://hal.in2p3.fr/in2p3-00368763 | |
| oai:hal.in2p3.fr:in2p3-00368763 | |
| Contributeur : Simone Lantz | |
| Soumis le : Mardi 17 Mars 2009, 15:29:07 | |
| Dernière modification le : Samedi 23 Juin 2012, 12:57:48 | |
