dc.creatorRomero, Gustavo Esteban
dc.creatorSotomayor Checa, Pablo Omar
dc.date.accessioned2019-08-28T18:29:00Z
dc.date.accessioned2022-10-15T01:30:49Z
dc.date.available2019-08-28T18:29:00Z
dc.date.available2022-10-15T01:30:49Z
dc.date.created2019-08-28T18:29:00Z
dc.date.issued2018-07
dc.identifierRomero, Gustavo Esteban; Sotomayor Checa, Pablo Omar; Population III microquasars; World Scientific; International Journal of Modern Physics D; 27; 10; 7-2018; 1-7
dc.identifier0218-2718
dc.identifierhttp://hdl.handle.net/11336/82402
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4330167
dc.description.abstractWe 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.
dc.languageeng
dc.publisherWorld Scientific
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1142/S0218271818440194
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.worldscientific.com/doi/abs/10.1142/S0218271818440194
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectBINARIES
dc.subjectDARK AGES
dc.subjectFIRST STARS
dc.subjectNONTHERMAL
dc.subjectRADIATION MECHANISMS
dc.subjectREIONIZATION
dc.subjectX-RAYS
dc.titlePopulation III microquasars
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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