Extreme photopolarimetric behaviour of the blazar AO 0235+164
- Autores
- Cellone, Sergio Aldo; Romero, Gustavo Esteban; Combi, Jorge Ariel; Martí, J.
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present optical photopolarimetric observations with high temporal resolution of the blazar AO 0235+164. Our data, the first to test the photopolarimetric behaviour of this object at very short time-scales, show significant micro-variability in total flux, colour index, linear polarization degree and position angle. Strong inter-night variations are also detected for these parameters. Although no correlation between colour index and total flux was found, our data seem to support the general bluer-when-brighter trend already known for this object. The polarization degree, in turn, shows no correlation with total flux, but a clear trend in the sense that colour index is redder (the spectrum is softer) when the measured polarization is higher.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
BL Lacertae objects: individual: AO 0235+164
Galaxies: active
Galaxies: photometry - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83157
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Extreme photopolarimetric behaviour of the blazar AO 0235+164Cellone, Sergio AldoRomero, Gustavo EstebanCombi, Jorge ArielMartí, J.Ciencias AstronómicasBL Lacertae objects: individual: AO 0235+164Galaxies: activeGalaxies: photometryWe present optical photopolarimetric observations with high temporal resolution of the blazar AO 0235+164. Our data, the first to test the photopolarimetric behaviour of this object at very short time-scales, show significant micro-variability in total flux, colour index, linear polarization degree and position angle. Strong inter-night variations are also detected for these parameters. Although no correlation between colour index and total flux was found, our data seem to support the general bluer-when-brighter trend already known for this object. The polarization degree, in turn, shows no correlation with total flux, but a clear trend in the sense that colour index is redder (the spectrum is softer) when the measured polarization is higher.Facultad de Ciencias Astronómicas y Geofísicas2007info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf60-64http://sedici.unlp.edu.ar/handle/10915/83157enginfo:eu-repo/semantics/altIdentifier/issn/1745-3933info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2007.00366.xinfo: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:UNLP2025-09-29T11:15:41Zoai:sedici.unlp.edu.ar:10915/83157Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:42.079SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
title |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
spellingShingle |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 Cellone, Sergio Aldo Ciencias Astronómicas BL Lacertae objects: individual: AO 0235+164 Galaxies: active Galaxies: photometry |
title_short |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
title_full |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
title_fullStr |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
title_full_unstemmed |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
title_sort |
Extreme photopolarimetric behaviour of the blazar AO 0235+164 |
dc.creator.none.fl_str_mv |
Cellone, Sergio Aldo Romero, Gustavo Esteban Combi, Jorge Ariel Martí, J. |
author |
Cellone, Sergio Aldo |
author_facet |
Cellone, Sergio Aldo Romero, Gustavo Esteban Combi, Jorge Ariel Martí, J. |
author_role |
author |
author2 |
Romero, Gustavo Esteban Combi, Jorge Ariel Martí, J. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas BL Lacertae objects: individual: AO 0235+164 Galaxies: active Galaxies: photometry |
topic |
Ciencias Astronómicas BL Lacertae objects: individual: AO 0235+164 Galaxies: active Galaxies: photometry |
dc.description.none.fl_txt_mv |
We present optical photopolarimetric observations with high temporal resolution of the blazar AO 0235+164. Our data, the first to test the photopolarimetric behaviour of this object at very short time-scales, show significant micro-variability in total flux, colour index, linear polarization degree and position angle. Strong inter-night variations are also detected for these parameters. Although no correlation between colour index and total flux was found, our data seem to support the general bluer-when-brighter trend already known for this object. The polarization degree, in turn, shows no correlation with total flux, but a clear trend in the sense that colour index is redder (the spectrum is softer) when the measured polarization is higher. Facultad de Ciencias Astronómicas y Geofísicas |
description |
We present optical photopolarimetric observations with high temporal resolution of the blazar AO 0235+164. Our data, the first to test the photopolarimetric behaviour of this object at very short time-scales, show significant micro-variability in total flux, colour index, linear polarization degree and position angle. Strong inter-night variations are also detected for these parameters. Although no correlation between colour index and total flux was found, our data seem to support the general bluer-when-brighter trend already known for this object. The polarization degree, in turn, shows no correlation with total flux, but a clear trend in the sense that colour index is redder (the spectrum is softer) when the measured polarization is higher. |
publishDate |
2007 |
dc.date.none.fl_str_mv |
2007 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/83157 |
url |
http://sedici.unlp.edu.ar/handle/10915/83157 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1745-3933 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2007.00366.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 60-64 |
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