Optical multicolor polarization observations in the region of the open cluster NGC 5749
- Autores
- Vergne, María Marcela; Feinstein Baigorri, Carlos; Martínez, Rubén Enrique
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present (UBVRI) multicolor linear polarimetric data for 31 of the brightest stars in the area of the open cluster NGC 5749 considered to study the properties of the interstellar medium (ISM) towards the cluster. Our data yield a mean polarization percentage of Pv ∼ 1.7%, close to the polarization value produced by the ISM with normal efficiency (P(%) = 3.5E (B-V)0.8) for a mean color excess of EB-V = 0.42. The mean angle of polarization vectors, θ = 74°, agrees quite well with the expected angle produced by dust particles aligned in the direction of the galactic disk (and the magnetic field) in the region. Our analysis indicates that the visual absorption affecting the stars in NGC 5749 is partially produced by a dust layer located up to 300 pc from the Sun and also by a second layer of dust closer to the cluster (located at least at 700 pc). The observed photometry and our polarization data are consistent with the existence of dust within the cluster. We also show in this work how polarimetry could be an excellent technique for identifying nonmember stars.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
ISM: dust, extinction
Open clusters and associations: individual: NGC 5749 - 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:10915/82966
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Optical multicolor polarization observations in the region of the open cluster NGC 5749Vergne, María MarcelaFeinstein Baigorri, CarlosMartínez, Rubén EnriqueCiencias AstronómicasISM: dust, extinctionOpen clusters and associations: individual: NGC 5749We present (UBVRI) multicolor linear polarimetric data for 31 of the brightest stars in the area of the open cluster NGC 5749 considered to study the properties of the interstellar medium (ISM) towards the cluster. Our data yield a mean polarization percentage of Pv ∼ 1.7%, close to the polarization value produced by the ISM with normal efficiency (P(%) = 3.5E (B-V)0.8) for a mean color excess of EB-V = 0.42. The mean angle of polarization vectors, θ = 74°, agrees quite well with the expected angle produced by dust particles aligned in the direction of the galactic disk (and the magnetic field) in the region. Our analysis indicates that the visual absorption affecting the stars in NGC 5749 is partially produced by a dust layer located up to 300 pc from the Sun and also by a second layer of dust closer to the cluster (located at least at 700 pc). The observed photometry and our polarization data are consistent with the existence of dust within the cluster. We also show in this work how polarimetry could be an excellent technique for identifying nonmember stars.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/pdf621-626http://sedici.unlp.edu.ar/handle/10915/82966enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20042124info: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:UNLP2025-09-29T11:15:45Zoai:sedici.unlp.edu.ar:10915/82966Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:45.875SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
title |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
spellingShingle |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 Vergne, María Marcela Ciencias Astronómicas ISM: dust, extinction Open clusters and associations: individual: NGC 5749 |
title_short |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
title_full |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
title_fullStr |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
title_full_unstemmed |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
title_sort |
Optical multicolor polarization observations in the region of the open cluster NGC 5749 |
dc.creator.none.fl_str_mv |
Vergne, María Marcela Feinstein Baigorri, Carlos Martínez, Rubén Enrique |
author |
Vergne, María Marcela |
author_facet |
Vergne, María Marcela Feinstein Baigorri, Carlos Martínez, Rubén Enrique |
author_role |
author |
author2 |
Feinstein Baigorri, Carlos Martínez, Rubén Enrique |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas ISM: dust, extinction Open clusters and associations: individual: NGC 5749 |
topic |
Ciencias Astronómicas ISM: dust, extinction Open clusters and associations: individual: NGC 5749 |
dc.description.none.fl_txt_mv |
We present (UBVRI) multicolor linear polarimetric data for 31 of the brightest stars in the area of the open cluster NGC 5749 considered to study the properties of the interstellar medium (ISM) towards the cluster. Our data yield a mean polarization percentage of Pv ∼ 1.7%, close to the polarization value produced by the ISM with normal efficiency (P(%) = 3.5E (B-V)0.8) for a mean color excess of EB-V = 0.42. The mean angle of polarization vectors, θ = 74°, agrees quite well with the expected angle produced by dust particles aligned in the direction of the galactic disk (and the magnetic field) in the region. Our analysis indicates that the visual absorption affecting the stars in NGC 5749 is partially produced by a dust layer located up to 300 pc from the Sun and also by a second layer of dust closer to the cluster (located at least at 700 pc). The observed photometry and our polarization data are consistent with the existence of dust within the cluster. We also show in this work how polarimetry could be an excellent technique for identifying nonmember stars. Facultad de Ciencias Astronómicas y Geofísicas |
description |
We present (UBVRI) multicolor linear polarimetric data for 31 of the brightest stars in the area of the open cluster NGC 5749 considered to study the properties of the interstellar medium (ISM) towards the cluster. Our data yield a mean polarization percentage of Pv ∼ 1.7%, close to the polarization value produced by the ISM with normal efficiency (P(%) = 3.5E (B-V)0.8) for a mean color excess of EB-V = 0.42. The mean angle of polarization vectors, θ = 74°, agrees quite well with the expected angle produced by dust particles aligned in the direction of the galactic disk (and the magnetic field) in the region. Our analysis indicates that the visual absorption affecting the stars in NGC 5749 is partially produced by a dust layer located up to 300 pc from the Sun and also by a second layer of dust closer to the cluster (located at least at 700 pc). The observed photometry and our polarization data are consistent with the existence of dust within the cluster. We also show in this work how polarimetry could be an excellent technique for identifying nonmember stars. |
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/10915/82966 |
url |
http://sedici.unlp.edu.ar/handle/10915/82966 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20042124 |
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) |
dc.format.none.fl_str_mv |
application/pdf 621-626 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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Universidad Nacional de La Plata |
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UNLP |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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