dc.creatorRomero, Gustavo Esteban
dc.creatorCombi, Jorge Ariel
dc.creatorVucetich, Héctor
dc.date1995
dc.date2022-11-15T13:45:15Z
dc.date.accessioned2023-07-15T05:04:28Z
dc.date.available2023-07-15T05:04:28Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/145833
dc.identifierissn:0004-640X
dc.identifierissn:1572-946X
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7471987
dc.descriptionWe present an intrinsic interpretation for the recently reported radio variability in the southern blazar PKS 0521-365. A shockedjet model can account for the quasi-periodical variations in the flux density of the source by means of inhomogeneities in the electron density with a quasi-periodic distribution along a jet in which a relativistic strong shock is propagating. These inhomogeneities are naturally produced by the effects of Kelvin-Helmholtz instabilities in the hypersonic parsec scale jet. The quasi-linear evolution of the polarization position angle can be understood as an effect of the “illumination” of successive cross sections with different mean field orientation or as a consequence of the shock propagation through a turbulent region in the jet. The high brightness temperature problem introduced by the short timescale varibility is solved invocating relativistic boosting with a moderately small viewing angle in agreement with the known structure of the source. In this context, several parameters are estimated.
dc.descriptionInstituto Argentino de Radioastronomía
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format183-204
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectBrightness temperature
dc.subjectPosition angle
dc.subjectShock propagation
dc.subjectPolarization position
dc.subjectField orientation
dc.titleRapid variability in the southern blazar PKS 0521-365
dc.typeArticulo
dc.typeArticulo


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