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dc.date.accessioned 2021-12-07T18:57:10Z
dc.date.available 2021-12-07T18:57:10Z
dc.date.issued 2021
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/129283
dc.description.abstract Binary systems of Population III can evolve to microquasars when one of the stars collapses into a black hole. When the compact object accretes matter at a rate greater than the Eddington rate, powerful jets and winds driven by strong radiation pressure should form. We investigate the structure of the jet-wind system for a model of Population III microquasar on scales beyond the jet-wind formation region. Using relativistic hydrodynamic simulations we find that the ratio of kinetic power between the jet and the disk wind determines the configuration of the system. When the power is dominated by the wind, the jet fills a narrow channel, collimated by the dense outflow. When the jet dominates the power of the system, part of its energy is diverted turning the wind into a quasi-equatorial flow, while the jet widens. From the results of our simulations, we implement semi-analytical calculations of the impact of the quasi-equatorial wind on scales of the order of the size of the binary system. Our results indicate that Population III microquasars might inject gamma rays and relativistic particles into the early intergalactic medium, contributing to its reionization at large distances from the binary system. en
dc.language en es
dc.subject Accretion, accretion disks es
dc.subject Stars: black holes es
dc.subject Stars: winds, outflows es
dc.subject Stars: Population III es
dc.subject X-rays: binaries es
dc.title Equatorial outflows driven by jets in Population III microquasars en
dc.type Articulo es
sedici.identifier.other doi:10.1007/s10509-020-03911-5 es
sedici.identifier.issn 0004-640X es
sedici.identifier.issn 1572-946X es
sedici.creator.person Sotomayor Checa, Pablo Omar es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Bosch-Ramon, Valentí es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astrophysics and Space Science es
sedici.relation.journalVolumeAndIssue vol. 366, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)