Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2021-09-15T18:57:31Z
dc.date.available 2021-09-15T18:57:31Z
dc.date.issued 2018
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/124902
dc.description.abstract We present the first results obtained in the elaboration of a complete model of a microquasar where the donor star is from Population III. These stars do not produce stellar winds so we consider that the mass loss is due exclusively to matter overflowing the Roche lobe towards the compact object, a maximally rotating black hole. The rate of accretion is extremely super-Eddington, with an intense mass loss from the system in the form of winds and jets. We calculate the relativistic particle content of the jet and the corresponding spectral energy distribution (SED) considering a lepto-hadronic model. Prospects for the cosmological implications of these objects are briefly discussed. en
dc.language en es
dc.subject Dark ages es
dc.subject Reionization es
dc.subject First stars es
dc.subject Radiation mechanisms: non-thermal es
dc.subject X-rays: binaries es
dc.title Population III microquasars en
dc.type Articulo es
sedici.identifier.other arXiv:1807.10157 es
sedici.identifier.other doi:10.1142/s0218271818440194 es
sedici.identifier.issn 0218-2718 es
sedici.identifier.issn 1793-6594 es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Sotomayor Checa, Pablo Omar es
sedici.subject.materias Ciencias Astronómicas es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle International Journal of Modern Physics D es
sedici.relation.journalVolumeAndIssue vol. 27, no. 10 es


Descargar archivos

Thumbnail
Documento
Descargar archivo (654.0Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)