Artículo
Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, G.; Castelletti, G.; Orlando, S.; Iakubovskyi, D.; Telezhinsky, I. "Predicted γ-ray image of SN 1006 due to inverse Compton emission" (2009) Monthly Notices of the Royal Astronomical Society. 399(1):157-165
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Abstract:
We propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC γ-ray images of SN 1006 show morphology in nice agreement with that reported by the High Energy Stereoscopic System (HESS) collaboration. The good correlation found between the observed very high energy γ-ray and X-ray/radio appearance can be considered as evidence of the fact that the γ-ray emission of SN 1006 observed by HESS is leptonic in origin, although a hadronic origin may not be excluded. © 2009 RAS.
Registro:
| Documento: | Artículo |
| Título: | Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| Autor: | Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, G.; Castelletti, G.; Orlando, S.; Iakubovskyi, D.; Telezhinsky, I. |
| Filiación: | Institute for Applied Problems in Mechanics and Mathematics, Naukova St. 3-b, 79060 Lviv, Ukraine National University, Kyryla and Methodia St. 8, 79008 Lviv, Ukraine Consorzio COMETA, Via S. Sofia 64, 95123 Catania, Italy INAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy Dipartimento di Scienze Fisiche Ed Astronomiche, Sezione di Astronomia, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy Instituto de Astronomía y Física Del Espacio (IAFE), CC 67, Suc. 28, 1428 Buenos Aires, Argentina Bogolyubov Institute for Theoretical Physics, Metrologichna St. 14-b, 03680 Kiev, Ukraine Kiev National Taras Shevchenko University, Observatorna St. 3, 04053 Kiev, Ukraine |
| Palabras clave: | Acceleration of particles; ISM: cosmic rays; ISM: individual: SN 1006; ISM: supernova remnants; Radiation mechanisms: non-thermal; Shock waves |
| Año: | 2009 |
| Volumen: | 399 |
| Número: | 1 |
| Página de inicio: | 157 |
| Página de fin: | 165 |
| DOI: | http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x |
| Título revista: | Monthly Notices of the Royal Astronomical Society |
| Título revista abreviado: | Mon. Not. R. Astron. Soc. |
| ISSN: | 00358711 |
| CODEN: | MNRAA |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v399_n1_p157_Petruk |
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Citas:
---------- APA ----------
Petruk, O., Bocchino, F., Miceli, M., Dubner, G., Castelletti, G., Orlando, S., Iakubovskyi, D.,..., Telezhinsky, I. (2009) . Predicted γ-ray image of SN 1006 due to inverse Compton emission. Monthly Notices of the Royal Astronomical Society, 399(1), 157-165.http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x
---------- CHICAGO ----------
Petruk, O., Bocchino, F., Miceli, M., Dubner, G., Castelletti, G., Orlando, S., et al. "Predicted γ-ray image of SN 1006 due to inverse Compton emission" . Monthly Notices of the Royal Astronomical Society 399, no. 1 (2009) : 157-165.http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x
---------- MLA ----------
Petruk, O., Bocchino, F., Miceli, M., Dubner, G., Castelletti, G., Orlando, S., et al. "Predicted γ-ray image of SN 1006 due to inverse Compton emission" . Monthly Notices of the Royal Astronomical Society, vol. 399, no. 1, 2009, pp. 157-165.http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x
---------- VANCOUVER ----------
Petruk, O., Bocchino, F., Miceli, M., Dubner, G., Castelletti, G., Orlando, S., et al. Predicted γ-ray image of SN 1006 due to inverse Compton emission. Mon. Not. R. Astron. Soc. 2009;399(1):157-165.http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x
