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dc.contributor.author
Vieyro, Florencia Laura  
dc.contributor.author
Bosch Ramon, Valentí  
dc.contributor.author
Torres Alba, Nuria  
dc.contributor.other
Aharonian, Felix A.  
dc.date.available
2021-08-20T02:45:22Z  
dc.date.issued
2018  
dc.identifier.citation
Non-thermal emission produced by the interaction of a jet with a supernova remnant; High-Energy Phenomena in Relativistic Outflows VI; Moscu; Rusia; 2017; 1-8  
dc.identifier.issn
0218-2718  
dc.identifier.uri
http://hdl.handle.net/11336/138579  
dc.description.abstract
Core-collapse supernovae (SNe) are found in galaxies with ongoing star-formation. If a starburst galaxy hosts an active galactic nucleus (AGN) with a relativistic jet, the SN could take place inside the jet. The collision of the SN ejecta with the jet flow leads to the formation of a shock, where particles could be accelerated up to relativistic energies, and produce gamma-ray emission. In this work, we analyze the dynamical evolution of the SN within the jet, and compute the non-thermal radiation expected from the interaction. The evolution of the SN Lorentz factor and radius regulates the intensity of the non-thermal emission. The SN can achieve a relativistic regime for powerful jets, resulting in emission significantly enhanced by Doppler boosting for blazar sources. The interaction of SNe with jets of moderate luminosity can result in steady, unbeamed gamma-ray emission, that might be detectable for sources in the local universe.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
World Scientific  
dc.rights
info:eu-repo/semantics/restrictedAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Relativistic jets  
dc.subject
Active Galactic Nuclei  
dc.subject
Non-thermal emission  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Non-thermal emission produced by the interaction of a jet with a supernova remnant  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.type
info:eu-repo/semantics/conferenceObject  
dc.type
info:ar-repo/semantics/documento de conferencia  
dc.date.updated
2021-07-01T16:56:05Z  
dc.identifier.eissn
1793-6594  
dc.journal.volume
27  
dc.journal.number
10  
dc.journal.pagination
1-8  
dc.journal.pais
Singapur  
dc.journal.ciudad
Singapur  
dc.description.fil
Fil: Vieyro, Florencia Laura. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad de Barcelona; España  
dc.description.fil
Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España  
dc.description.fil
Fil: Torres Alba, Nuria. Universidad de Barcelona; España  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://dx.doi.org/10.1142/S0218271818440212  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://hepro6.cosmos.ru/  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://hepro6.cosmos.ru/sites/hepro6.cosmos.ru/files/hepro6_program.pdf  
dc.conicet.rol
Autor  
dc.conicet.rol
Autor  
dc.conicet.rol
Autor  
dc.coverage
Internacional  
dc.type.subtype
Conferencia  
dc.description.nombreEvento
High-Energy Phenomena in Relativistic Outflows VI  
dc.date.evento
2017-09-11  
dc.description.ciudadEvento
Moscu  
dc.description.paisEvento
Rusia  
dc.type.publicacion
Journal  
dc.description.institucionOrganizadora
Space Research Institute of Russian Academy of Sciences  
dc.source.revista
International Journal of Modern Physics D  
dc.date.eventoHasta
2017-09-15  
dc.type
Conferencia