A massive binary system can feed Sgr A*

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dc.contributor.authorCalderón Espinoza, Diego Nicolás
dc.contributor.authorCuadra, Jorge
dc.date.accessioned2020-04-20T19:35:04Z
dc.date.available2020-04-20T19:35:04Z
dc.date.issued2017
dc.date.updated2020-04-09T20:17:16Z
dc.description.abstractThe enigmatic G2 cloud just passed pericentre around the Galactic Centre super-massive black hole, Sgr A. Despite all theoretical and observational efforts, its nature remains unclear. If purely gaseous, it is possible to explain it as a gas clump formed in a colliding wind binary. Here we study the hypothesis of G2 being one of such clumps ejected from the massive binary IRS 16SW....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/28688
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/2017RMxAC..49..101C/abstract
dc.language.isoen
dc.nota.accesoContenido parcial
dc.relation.isformatofLatin American Regional IAU Meeting Cartagena 2016 (15o. : 2016 : Cartajena de Indias, Colombia)
dc.revistaRevista Mexicana de Astronomia y Astrofisica Conference Serieses_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxiaes_ES
dc.subject.otherGalaxias - Evoluciónes_ES
dc.subject.otherAgujeros negroses_ES
dc.titleA massive binary system can feed Sgr A*es_ES
dc.typecomunicación de congreso
sipa.codpersvinculados224673
sipa.codpersvinculados3855
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