Microvariability in the optical polarization of 3C 279
- Autores
- Andruchow, Ileana; Cellone, Sergio Aldo; Romero, Gustavo Esteban; Dominici, T. P.; Abraham, Z.
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Galaxies: active
Galaxies: individual: 3C 279
Galaxies: photometry
Polarization - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84492
Ver los metadatos del registro completo
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Microvariability in the optical polarization of 3C 279Andruchow, IleanaCellone, Sergio AldoRomero, Gustavo EstebanDominici, T. P.Abraham, Z.Ciencias AstronómicasGalaxies: activeGalaxies: individual: 3C 279Galaxies: photometryPolarizationWe 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.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2003info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf857-865http://sedici.unlp.edu.ar/handle/10915/84492enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20031178info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-11-12T10:40:32Zoai:sedici.unlp.edu.ar:10915/84492Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-11-12 10:40:33.228SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Microvariability in the optical polarization of 3C 279 |
| title |
Microvariability in the optical polarization of 3C 279 |
| spellingShingle |
Microvariability in the optical polarization of 3C 279 Andruchow, Ileana Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization |
| title_short |
Microvariability in the optical polarization of 3C 279 |
| title_full |
Microvariability in the optical polarization of 3C 279 |
| title_fullStr |
Microvariability in the optical polarization of 3C 279 |
| title_full_unstemmed |
Microvariability in the optical polarization of 3C 279 |
| title_sort |
Microvariability in the optical polarization of 3C 279 |
| dc.creator.none.fl_str_mv |
Andruchow, Ileana Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. |
| author |
Andruchow, Ileana |
| author_facet |
Andruchow, Ileana Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. |
| author_role |
author |
| author2 |
Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. |
| author2_role |
author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization |
| topic |
Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization |
| dc.description.none.fl_txt_mv |
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. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
| description |
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. |
| publishDate |
2003 |
| dc.date.none.fl_str_mv |
2003 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/84492 |
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http://sedici.unlp.edu.ar/handle/10915/84492 |
| dc.language.none.fl_str_mv |
eng |
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eng |
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