Predicted γ-ray image of SN 1006 due to inverse Compton emission
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 S...
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todo:paper_00358711_v399_n1_p157_Petruk2023-10-03T14:46:56Z Predicted γ-ray image of SN 1006 due to inverse Compton emission Petruk, O. Bocchino, F. Miceli, M. Dubner, G. Castelletti, G. Orlando, S. Iakubovskyi, D. Telezhinsky, I. Acceleration of particles ISM: cosmic rays ISM: individual: SN 1006 ISM: supernova remnants Radiation mechanisms: non-thermal Shock waves 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v399_n1_p157_Petruk |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Acceleration of particles ISM: cosmic rays ISM: individual: SN 1006 ISM: supernova remnants Radiation mechanisms: non-thermal Shock waves |
| spellingShingle |
Acceleration of particles ISM: cosmic rays ISM: individual: SN 1006 ISM: supernova remnants Radiation mechanisms: non-thermal Shock waves 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 |
| topic_facet |
Acceleration of particles ISM: cosmic rays ISM: individual: SN 1006 ISM: supernova remnants Radiation mechanisms: non-thermal Shock waves |
| description |
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. |
| format |
JOUR |
| author |
Petruk, O. Bocchino, F. Miceli, M. Dubner, G. Castelletti, G. Orlando, S. Iakubovskyi, D. Telezhinsky, I. |
| author_facet |
Petruk, O. Bocchino, F. Miceli, M. Dubner, G. Castelletti, G. Orlando, S. Iakubovskyi, D. Telezhinsky, I. |
| author_sort |
Petruk, O. |
| title |
Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| title_short |
Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| title_full |
Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| title_fullStr |
Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| title_full_unstemmed |
Predicted γ-ray image of SN 1006 due to inverse Compton emission |
| title_sort |
predicted γ-ray image of sn 1006 due to inverse compton emission |
| url |
http://hdl.handle.net/20.500.12110/paper_00358711_v399_n1_p157_Petruk |
| work_keys_str_mv |
AT petruko predictedgrayimageofsn1006duetoinversecomptonemission AT bocchinof predictedgrayimageofsn1006duetoinversecomptonemission AT micelim predictedgrayimageofsn1006duetoinversecomptonemission AT dubnerg predictedgrayimageofsn1006duetoinversecomptonemission AT castellettig predictedgrayimageofsn1006duetoinversecomptonemission AT orlandos predictedgrayimageofsn1006duetoinversecomptonemission AT iakubovskyid predictedgrayimageofsn1006duetoinversecomptonemission AT telezhinskyi predictedgrayimageofsn1006duetoinversecomptonemission |
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