Microvariability in the optical polarization of 3C 279
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 consistin...
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| Autores principales: | , , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2003
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84492 |
| Aporte de: |
| id |
I19-R120-10915-84492 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization |
| spellingShingle |
Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization Andruchow, Ileana Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. Microvariability in the optical polarization of 3C 279 |
| topic_facet |
Ciencias Astronómicas Galaxies: active Galaxies: individual: 3C 279 Galaxies: photometry Polarization |
| 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. |
| format |
Articulo Articulo |
| author |
Andruchow, Ileana Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. |
| author_facet |
Andruchow, Ileana Cellone, Sergio Aldo Romero, Gustavo Esteban Dominici, T. P. Abraham, Z. |
| author_sort |
Andruchow, Ileana |
| title |
Microvariability in the optical polarization of 3C 279 |
| 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 |
| publishDate |
2003 |
| url |
http://sedici.unlp.edu.ar/handle/10915/84492 |
| work_keys_str_mv |
AT andruchowileana microvariabilityintheopticalpolarizationof3c279 AT cellonesergioaldo microvariabilityintheopticalpolarizationof3c279 AT romerogustavoesteban microvariabilityintheopticalpolarizationof3c279 AT dominicitp microvariabilityintheopticalpolarizationof3c279 AT abrahamz microvariabilityintheopticalpolarizationof3c279 |
| bdutipo_str |
Repositorios |
| _version_ |
1764820488790474754 |