A search for disks around exoplanet host stars
- Autores
- Saffe, Carlos; Gómez, M.
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We have assembled a database which comprises optical and infrared (IR) photometry of Exoplanet Host stars (EHs), and constructed the spectral energy distributions (SEDs) of these stars. We use several quantities to explore the existence of excess IR emission with respect to the photospheric level. In particular, the criteria proposed by Manning & Barlow (1998) identify IR excess in 19-23% of the class V EH sources (i.e., in 6-7 out of 31). Several searches for Vega-like systems have yielded a similar fraction of objects with IR excess emission among main sequence stars. This excess emission is likely due to the presence of dust in circumstellar disks. We compare the optical polarization properties of the EHs, Vega-like candidate objects and pre-main sequence stars. While the median polarizations of the EHs and Vega-like candidate objects are very similar, both groups have significant lower median optical polarization values than T Tauri and Herbig AeBe stars.
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Gómez, M.. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina - Materia
-
STARS: CIRCUMSTELLA MATTER
STARS: PLANETARY SYSTEMS
TECHNIQUE: PHOTOMETRY
TECHNIQUE: POLARIMETRY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/241758
Ver los metadatos del registro completo
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A search for disks around exoplanet host starsSaffe, CarlosGómez, M.STARS: CIRCUMSTELLA MATTERSTARS: PLANETARY SYSTEMSTECHNIQUE: PHOTOMETRYTECHNIQUE: POLARIMETRYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We have assembled a database which comprises optical and infrared (IR) photometry of Exoplanet Host stars (EHs), and constructed the spectral energy distributions (SEDs) of these stars. We use several quantities to explore the existence of excess IR emission with respect to the photospheric level. In particular, the criteria proposed by Manning & Barlow (1998) identify IR excess in 19-23% of the class V EH sources (i.e., in 6-7 out of 31). Several searches for Vega-like systems have yielded a similar fraction of objects with IR excess emission among main sequence stars. This excess emission is likely due to the presence of dust in circumstellar disks. We compare the optical polarization properties of the EHs, Vega-like candidate objects and pre-main sequence stars. While the median polarizations of the EHs and Vega-like candidate objects are very similar, both groups have significant lower median optical polarization values than T Tauri and Herbig AeBe stars.Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Gómez, M.. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaEDP Sciences2004-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/241758Saffe, Carlos; Gómez, M.; A search for disks around exoplanet host stars; EDP Sciences; Astronomy and Astrophysics; 423; 1; 7-2004; 221-2330004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2004/31/aa0241-04/aa0241-04.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20040241info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:45:26Zoai:ri.conicet.gov.ar:11336/241758instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:45:27.19CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A search for disks around exoplanet host stars |
title |
A search for disks around exoplanet host stars |
spellingShingle |
A search for disks around exoplanet host stars Saffe, Carlos STARS: CIRCUMSTELLA MATTER STARS: PLANETARY SYSTEMS TECHNIQUE: PHOTOMETRY TECHNIQUE: POLARIMETRY |
title_short |
A search for disks around exoplanet host stars |
title_full |
A search for disks around exoplanet host stars |
title_fullStr |
A search for disks around exoplanet host stars |
title_full_unstemmed |
A search for disks around exoplanet host stars |
title_sort |
A search for disks around exoplanet host stars |
dc.creator.none.fl_str_mv |
Saffe, Carlos Gómez, M. |
author |
Saffe, Carlos |
author_facet |
Saffe, Carlos Gómez, M. |
author_role |
author |
author2 |
Gómez, M. |
author2_role |
author |
dc.subject.none.fl_str_mv |
STARS: CIRCUMSTELLA MATTER STARS: PLANETARY SYSTEMS TECHNIQUE: PHOTOMETRY TECHNIQUE: POLARIMETRY |
topic |
STARS: CIRCUMSTELLA MATTER STARS: PLANETARY SYSTEMS TECHNIQUE: PHOTOMETRY TECHNIQUE: POLARIMETRY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We have assembled a database which comprises optical and infrared (IR) photometry of Exoplanet Host stars (EHs), and constructed the spectral energy distributions (SEDs) of these stars. We use several quantities to explore the existence of excess IR emission with respect to the photospheric level. In particular, the criteria proposed by Manning & Barlow (1998) identify IR excess in 19-23% of the class V EH sources (i.e., in 6-7 out of 31). Several searches for Vega-like systems have yielded a similar fraction of objects with IR excess emission among main sequence stars. This excess emission is likely due to the presence of dust in circumstellar disks. We compare the optical polarization properties of the EHs, Vega-like candidate objects and pre-main sequence stars. While the median polarizations of the EHs and Vega-like candidate objects are very similar, both groups have significant lower median optical polarization values than T Tauri and Herbig AeBe stars. Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina Fil: Gómez, M.. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina |
description |
We have assembled a database which comprises optical and infrared (IR) photometry of Exoplanet Host stars (EHs), and constructed the spectral energy distributions (SEDs) of these stars. We use several quantities to explore the existence of excess IR emission with respect to the photospheric level. In particular, the criteria proposed by Manning & Barlow (1998) identify IR excess in 19-23% of the class V EH sources (i.e., in 6-7 out of 31). Several searches for Vega-like systems have yielded a similar fraction of objects with IR excess emission among main sequence stars. This excess emission is likely due to the presence of dust in circumstellar disks. We compare the optical polarization properties of the EHs, Vega-like candidate objects and pre-main sequence stars. While the median polarizations of the EHs and Vega-like candidate objects are very similar, both groups have significant lower median optical polarization values than T Tauri and Herbig AeBe stars. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-07 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/241758 Saffe, Carlos; Gómez, M.; A search for disks around exoplanet host stars; EDP Sciences; Astronomy and Astrophysics; 423; 1; 7-2004; 221-233 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/241758 |
identifier_str_mv |
Saffe, Carlos; Gómez, M.; A search for disks around exoplanet host stars; EDP Sciences; Astronomy and Astrophysics; 423; 1; 7-2004; 221-233 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2004/31/aa0241-04/aa0241-04.html info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20040241 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614494195548160 |
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13.070432 |