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dc.contributor.authorMirabel, I. Felixpt_BR
dc.contributor.authorRodrigues, Irapuanpt_BR
dc.contributor.authorLiu, Q. Z.pt_BR
dc.date.accessioned2014-07-26T02:09:15Zpt_BR
dc.date.issued2004pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98761pt_BR
dc.description.abstractWe show that the microquasar LS I +61° 303 is running away from its birth place in a young complex of massive stars. The supernova explosion that formed the compact object shot out the X-ray binary with a linear momentum of 430 ± 140 Mѳ km sˉ¹, which is comparable to the linear momenta found in solitary runaway neutron stars and millisecond pulsars. The properties of the binary system and its runaway motion of 27±6 km sˉ¹ imply that the natal supernova was asymmetric and that the upper limit for the mass that could have been suddenly ejected in the explosion is ~2 Mѳ. The initial mass of the progenitor star of the compact object that is inferred depends on whether the formation of massive stars in the parent stellar cluster was coeval or a sequential process.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. Berlin. Vol. 422, no. 2 (Aug. 2004), p. L29-32pt_BR
dc.rightsOpen Accessen
dc.subjectFormacao de estrelaspt_BR
dc.subjectStars: individual: LS I +61° 303, 2CG 135+01, 3EG J0241+6103en
dc.subjectX-rays: binaries: starsen
dc.subjectBuracos negrospt_BR
dc.subjectGamma-rays: observationsen
dc.subjectEstrelas de neutronspt_BR
dc.subjectGamma-rays: theoryen
dc.subjectMassa estelarpt_BR
dc.subjectMovimento estelarpt_BR
dc.subjectMomento linearpt_BR
dc.subjectSupernovapt_BR
dc.subjectAglomerados estelarespt_BR
dc.titleA microquasar shot out from its birth placept_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000504458pt_BR
dc.type.originEstrangeiropt_BR


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