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dc.contributor.author
Bordas, Pol
dc.contributor.author
Paredes, Josep Maria
dc.contributor.author
Bosch Ramon, Valentí
dc.contributor.author
Orellana, Mariana Dominga
dc.date.available
2017-11-08T14:14:19Z
dc.date.issued
2007-04
dc.identifier.citation
Bordas, Pol; Paredes, Josep Maria; Bosch Ramon, Valentí; Orellana, Mariana Dominga; Synchrotron emission from secondary leptons in microquasar jets ; Springer; Astrophysics And Space Science; 309; 1-4; 4-2007; 339-343
dc.identifier.issn
0004-640X
dc.identifier.uri
http://hdl.handle.net/11336/27803
dc.description.abstract
We present a model to estimate the synchrotron radio emission generated in microquasar (MQ) jets due to secondary pairs created via decay of charged pions produced in proton-proton collisions between stellar wind ions and jet relativistic protons. The synchrotron radiation produced by secondary electrons/positrons is computed using consistently derived particle energy distributions. Energy losses due to synchrotron and inverse Compton (IC) processes, and adiabatic expansion, are taken into account. The space parameter for the model is explored and the corresponding spectral energy distributions (SEDs) are presented. We conclude that secondary leptonic emission represents a significant though hardly dominant contribution to the total radio emission in MQs, with observational consequences that can be used to test some still unknown processes occurring in these objects as well as the nature of the matter outflowing in their jets.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Springer
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Microquasars
dc.subject
Radio Emission
dc.subject
Secondary Leptons
dc.subject.classification
Astronomía
dc.subject.classification
Ciencias Físicas
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
dc.title
Synchrotron emission from secondary leptons in microquasar jets
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-10-12T19:38:22Z
dc.identifier.eissn
1572-946X
dc.journal.volume
309
dc.journal.number
1-4
dc.journal.pagination
339-343
dc.journal.pais
Alemania
dc.journal.ciudad
Berlin
dc.description.fil
Fil: Bordas, Pol. Universidad de Barcelona; España
dc.description.fil
Fil: Paredes, Josep Maria. Universidad de Barcelona; España. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
dc.description.fil
Fil: Bosch Ramon, Valentí. Max-Planck Institut für Kernphysik; Alemania
dc.description.fil
Fil: Orellana, Mariana Dominga. 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.journal.title
Astrophysics And Space Science
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://link.springer.com/article/10.1007%2Fs10509-007-9403-1
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s10509-007-9403-1


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