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dc.date.accessioned | 2019-10-31T13:45:26Z | |
dc.date.available | 2019-10-31T13:45:26Z | |
dc.date.issued | 2003 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/84492 | |
dc.description.abstract | We present results of a microvariability polarization study in the violently variable quasaer 3C279. We have resolved the polarization curves in the V band for this object down to timescales of minutes. We found two main components in the evolution of the degree of linear polarization, one consisting of a flicker with timescales of several tens of minutes and other component with far more significant variations on timescales of a few days. The linear polarization descended from ∼17%. down to ∼8% in three nights. The polarization angle underwent a sudden change of more that 10 degrees in a few hours, perhaps indicating the injection of a new shock in the jet. The amplitude of the intranight flickering in the degree of polarization is at the level of ∼1%. These are probably the best sampled polarization data ever obtained for this object. We also performed IR observations and we provide a follow-up of the evolution of this source at such energies after the main polarization outburst. | en |
dc.format.extent | 857-865 | es |
dc.language | en | es |
dc.subject | Galaxies: active | es |
dc.subject | Galaxies: individual: 3C 279 | es |
dc.subject | Galaxies: photometry | es |
dc.subject | Polarization | es |
dc.title | Microvariability in the optical polarization of 3C 279 | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1051/0004-6361:20031178 | es |
sedici.identifier.other | eid:2-s2.0-0142039968 | es |
sedici.identifier.issn | 0004-6361 | es |
sedici.creator.person | Andruchow, Ileana | es |
sedici.creator.person | Cellone, Sergio Aldo | es |
sedici.creator.person | Romero, Gustavo Esteban | es |
sedici.creator.person | Dominici, T. P. | es |
sedici.creator.person | Abraham, Z. | es |
sedici.subject.materias | Ciencias Astronómicas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Facultad de Ciencias Astronómicas y Geofísicas | es |
mods.originInfo.place | Instituto Argentino de Radioastronomía | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Astronomy and Astrophysics | es |
sedici.relation.journalVolumeAndIssue | vol. 409, no. 3 | es |
sedici.rights.sherpa | * RoMEO: verde* Pre-print del autor: can* Post-print del autor: can* Versión de editor/PDF:can* Condiciones:>>En el sitio web del autor o institucional o sitios que cumplan las directrices OAI>>Algunas revistas requieren un periodo de embargo para su depósito en repositorios recomendados por los organismos financiadores (ver revista)>>La versión de editor/PDF puede utilizarse (ver revista)>>Debe ir enlazado a la versión de editor>>Deben reconocerse el copyright y la fuente editorial>>No comercial* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0004-6361/es/ |