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dc.contributor.author
Vieyro, Florencia Laura
dc.contributor.author
Torres Alba, Nuria
dc.contributor.author
Bosch Ramon, Valentí
dc.contributor.other
Aharonian, Felix A.
dc.date.available
2021-08-20T03:29:21Z
dc.date.issued
2017
dc.identifier.citation
Non-thermal emission from the interaction of extragalactic jets with stars; 6th International Symposium on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2016; 1-6
dc.identifier.isbn
978-0-7354-1456-3
dc.identifier.issn
1551-7616
dc.identifier.uri
http://hdl.handle.net/11336/138592
dc.description.abstract
The central regions of galaxies are rich environments, with abundant stars and medium inhomogeneities. For galaxies hostingactive galactic nuclei, the interaction of a relativistic jet with obstacles can lead to the formation of shocks, where particles canbe accelerated up to relativistic energies. In this work, we analyze the non-thermal radiation produced by electrons accelerated inthese shocks. We first characterize the stellar population inside the jet. Then, we study the transport of relativistic electrons, andcompute their synchrotron and inverse Compton emission. In particular, we focus our research on AGN jets aligned with the lineof sight, where the observed emission is significantly enhanced by Doppler boosting.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
AIP Publishing
dc.rights
info:eu-repo/semantics/restrictedAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Processes: non-thermal
dc.subject
Relativistic jets
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Non-thermal emission from the interaction of extragalactic jets with stars
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
2021-07-01T16:55:54Z
dc.journal.volume
1792
dc.journal.number
1
dc.journal.pagination
1-6
dc.journal.pais
Estados Unidos
dc.journal.ciudad
New York
dc.description.fil
Fil: Vieyro, Florencia Laura. Universidad de Barcelona; España. 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
dc.description.fil
Fil: Torres Alba, Nuria. Universidad de Barcelona; España
dc.description.fil
Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://aip.scitation.org/doi/abs/10.1063/1.4968884
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1063/1.4968958
dc.conicet.rol
Autor
dc.conicet.rol
Autor
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Autor
dc.coverage
Internacional
dc.type.subtype
Simposio
dc.description.nombreEvento
6th International Symposium on High Energy Gamma-Ray Astronomy
dc.date.evento
2016-07-11
dc.description.ciudadEvento
Heidelberg
dc.description.paisEvento
Alemania
dc.type.publicacion
Journal
dc.description.institucionOrganizadora
Max-Planck-Institut für Nuclear Physics
dc.source.revista
AIP Conference Proceedings
dc.date.eventoHasta
2016-07-15
dc.type
Simposio
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