Giacani, E. and Rovero, A.C. (2001) Radio observations of a Galactic high energy gamma ray source. Il nuovo cimento C, 24 C (4\5). pp. 657-660. ISSN 1826-9885
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Abstract
PSR B1706-44 is one of the very few galactic pulsars that has been discovered at TeV energies. PSR B1706-44 has been also detected in the X-ray domain. It has been suggested that the high energy radiation could be due to inverse Compton radiation from a pulsar wind nebula (PWN). We report on VLA high-resolution observations of a region around the pulsar PSR B1706-44 at 1.4, 4.8 and 8.4 GHz. The pulsar appears embedded in a synchrotron nebula. We propose that this synchrotron nebula is the radio counterpart of the high energy emission powered by the spin-down energy of the pulsar.
| Item Type: | Article |
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| Additional Information: | aper presented at the Chacaltaya Meeting on Cosmic Ray Physics, La Paz, Bolivia, July 23-27, 2000. |
| Uncontrolled Keywords: | Cosmic rays ; Conference proceedings |
| Subjects: | 500 Scienze naturali e Matematica > 550 Scienze della Terra > 551 Geologia, Idrologia, Meteorologia > 551.5 Meteorologia (Classificare qui l'atmosfera) (Classificare la previsione e le previsioni di specifici fenomeni meteorologici in 551.64; classificare la Micrometeorologia in 551.66) > 551.52 Termodinamica, interazioni atmosferiche con la superficie terrestre, temperature, radiazioni > 551.527 Radiazioni (per fenomeni ottici, vedi 551.565) > 551.5276 Radiazioni cosmiche (Include il rumore cosmico) (Classificare qui i raggi cosmici) |
| Depositing User: | Marina Spanti |
| Date Deposited: | 11 Mar 2020 11:17 |
| Last Modified: | 11 Mar 2020 11:17 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/14515 |
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