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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  
dc.subject.classification
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