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dc.contributor.author
Torres Alba, Nuria
dc.contributor.author
Bosch Ramon, Valentí
dc.contributor.author
Vieyro, Florencia Laura
dc.contributor.other
Aharonian, Felix A.
dc.date.available
2021-08-20T03:30:47Z
dc.date.issued
2017
dc.identifier.citation
Characterizing the stellar populations interacting with AGN jets; 6th International Symposium on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2016; 1-5
dc.identifier.isbn
978-0-7354-1456-3
dc.identifier.issn
1551-7616
dc.identifier.uri
http://hdl.handle.net/11336/138593
dc.description.abstract
Galaxies hosting an active galactic nucleus may present interactions between relativistic jets, if present, and the surroundingmedium, especially if the central regions are rich in stars and gas. In particular, the presence of stars with strong windsentering into the jets can lead to the formation of shocks in which particles can be accelerated up to relativistic energies. Galaxieswith ongoing starbursts in the innermost regions will present a significant amount of young OB stars close to the central engine,whereas in older galaxies like M87 the population responsible for most of the jet-star interactions will be formed by red giants. Inthis work, we develop prescriptions for the spatial and mass distributions of different populations of stars inside AGN jets, and forthe mass-loss properties of these stars. Our final objective is to explore the consequences of such interactions for jet dynamics andradiation.
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
Relativistic jets
dc.subject
Starbursts
dc.subject
Stellar winds
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Characterizing the stellar populations interacting with AGN jets
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
2021-07-01T16:55:51Z
dc.journal.volume
1792
dc.journal.number
1
dc.journal.pagination
1-5
dc.journal.pais
Estados Unidos
dc.journal.ciudad
New York
dc.description.fil
Fil: Torres Alba, Nuria. Universidad de Barcelona; España
dc.description.fil
Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España
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.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/doi/https://doi.org/10.1063/1.4968884
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4968958
dc.conicet.rol
Autor
dc.conicet.rol
Autor
dc.conicet.rol
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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