Mostrar el registro sencillo del ítem

dc.contributor.author
Petruk, O.  
dc.contributor.author
Bocchino, F.  
dc.contributor.author
Miceli, M.  
dc.contributor.author
Dubner, Gloria Mabel  
dc.contributor.author
Castelletti, Gabriela Marta  
dc.contributor.author
Orlando, S.  
dc.contributor.author
Iakubovskyi, D.  
dc.contributor.author
Telezhinsky, I.  
dc.date.available
2017-08-04T21:25:20Z  
dc.date.issued
2009-12  
dc.identifier.citation
Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta; et al.; Predicted gamma-ray image of SN 1006 due to inverse Compton emission; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 399; 1; 12-2009; 157-165  
dc.identifier.issn
0035-8711  
dc.identifier.uri
http://hdl.handle.net/11336/21922  
dc.description.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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Oxford University Press  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Acceleration of Particles  
dc.subject
Ism: Cosmic Rays  
dc.subject
Ism: Individual: Sn 1006  
dc.subject
Ism: Supernova Remnants  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Predicted gamma-ray image of SN 1006 due to inverse Compton emission  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2017-07-28T15:06:29Z  
dc.journal.volume
399  
dc.journal.number
1  
dc.journal.pagination
157-165  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: Petruk, O.. Institute for Applied Problems in Mechanics and Mathematics; Ucrania  
dc.description.fil
Fil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia  
dc.description.fil
Fil: Miceli, M.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia  
dc.description.fil
Fil: Dubner, Gloria Mabel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina  
dc.description.fil
Fil: Castelletti, Gabriela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina  
dc.description.fil
Fil: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia  
dc.description.fil
Fil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; Ucrania  
dc.description.fil
Fil: Telezhinsky, I.. Kiev National Taras Shevchenko University; Ucrania  
dc.journal.title
Monthly Notices of the Royal Astronomical Society  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2009.15352.x  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1111/j.1365-2966.2009.15352.x  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0907.0976?context=astro-ph  

Archivos asociados
Thumbnail
 
Tamaño: 3.908Mb
Formato: PDF
.