Clump formation through colliding stellar winds in the Galactic Centre

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dc.contributor.authorCalderón Espinoza, Diego Nicolás
dc.contributor.authorBallone, A.
dc.contributor.authorCuadra, Jorge
dc.contributor.authorSchartmann, Marc
dc.contributor.authorBurkert, A.
dc.contributor.authorGillessen, S.
dc.date.accessioned2020-04-20T19:35:08Z
dc.date.available2020-04-20T19:35:08Z
dc.date.issued2017
dc.date.updated2020-04-09T20:17:33Z
dc.description.abstractWe study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW....
dc.fuente.origenORCID
dc.identifier.doi10.1017/S1743921316012011
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/28689
dc.identifier.urihttps://doi.org/10.1017/S1743921316012011
dc.language.isoen
dc.nota.accesoContenido parcial
dc.relation.isformatofLatin American Regional IAU Meeting Cartagena 2016 (15o. : 2016 : Cartajena de Indias, Colombia)
dc.revistaThe Multi-Messenger Astrophysics of the Galactic Centrees_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherHidrodinámicaes_ES
dc.subject.otherEstrellases_ES
dc.subject.otherGalaxiaes_ES
dc.titleClump formation through colliding stellar winds in the Galactic Centrees_ES
dc.typecomunicación de congreso
dc.volumenVol. 49
sipa.codpersvinculados224673
sipa.codpersvinculados3855
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