Analysis of the velocity data of cluster A562

dc.contributor.authorCalderón Espinoza, Diego Nicolás
dc.contributor.authorGómez, P.
dc.date.accessioned2020-04-20T19:35:13Z
dc.date.available2020-04-20T19:35:13Z
dc.date.issued2014
dc.date.updated2020-04-09T20:17:52Z
dc.description.abstractWe present a recent study of the dynamics of the cluster of galaxies Abell 562 intended to determine if ram pressure is responsible for the jet bending in the Wide-Angle Tailed (WAT) radio source located in the central elliptical galaxy. Given the properties of the jet and of the intra-cluster medium (ICM), a relative velocity between the galaxy and the ICM greater than 800 km/s is needed for this mechanism to bend the WAT jet. We find that the peculiar velocity of the WAT galaxy is 170 ± 140 km/s which is not enough to produce the bending. This is based on the analysis of the velocity of 146 galaxy cluster members obtained with the Gemini Multi-Object Spectrometer (GMOS) at Gemini North. However, our analysis of these velocity data and archival Chandra data suggests that an off-axis merger occurred in this system. This type of merger typically produces bulk flow motions with peak velocities greater than 1000 km/s which should be enough to explain the bending of the jets....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/28690
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/2014RMxAC..44..172C/abstract
dc.language.isoen
dc.nota.accesoContenido parcial
dc.relation.isformatofLatin American Regional IAU Meeting (14o. : 2013 : Florianópolis, SC, Brazil)
dc.revistaRevista Mexicana de Astronomia y Astrofisica Conference Serieses_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxias - Cúmuloses_ES
dc.subject.otherGalaxias - Espectroses_ES
dc.subject.otherGalaxias - Observacioneses_ES
dc.titleAnalysis of the velocity data of cluster A562es_ES
dc.typecomunicación de congreso
sipa.codpersvinculados224673
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