A temperature condensation trend in the debris-disk binary system ζ2 Ret

Autores
Saffe, Carlos; Flores Trivigno, Matias Gaston; Jaque Arancibia, Marcelo Daniel; Buccino, Andrea Paola; Jofre, Jorge Emiliano
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We explore condensation temperature Tc trends in the unique binary systemZet1 Ret - Zet2 Ret, to determine whether there is a depletion of refractories,which could be related to the planet formation process. The star Zet2 Ret hostsa debris disk which was detected by an IR excess and confirmed by directimaging and numerical simulations, while Zet1 Ret does not present IR excessnor planets. We carried out a high-precision abundance determination in bothcomponents of the binary system via a line-by-line, strictly differentialapproach. The stellar parameters Teff , log g, [Fe/H] and vturb were determinedby imposing differential ionization and excitation equilibrium of Fe I and FeII lines, with an updated version of the program FUNDPAR. The star Zet1 Retresulted slightly more metal rich than Zet2 Ret by 0.02 dex. In thedifferential calculation of Zet1 Ret using Zet2 Ret as reference, theabundances of the refractory elements resulted higher than the volatileelements, and the trend of the refractory elements with Tc showed a positiveslope. These facts together show a lack of refractory elements in Zet2 Ret (adebris-disk host) relative to Zet1 Ret. The Tc trend would be in agreement withthe proposed signature of planet formation (Melendez et al. 2009) rather thanpossible Galactic Chemical Evolution or age effects, which are largelydiminished here. Then, following the interpretation of Melendez et al. (2009),we propose an scenario in which the refractory elements depleted in Zet2 Retare possibly locked-up in the rocky material that orbits this star and producethe debris disk observed around this object. We estimated a lower limit ofMrock = 3 Me for the rocky mass of depleted material, which is compatible witha rough estimation of 3-50 Me of a debris disk mass around a solar-type star.
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geología; Argentina
Fil: Flores Trivigno, Matias Gaston. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Buccino, Andrea Paola. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
Fil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Materia
Stars: abundances
Stars: planetary systems
Stars: binaries
tars: individual: ζ 1 Ret ( = HD 20766), ζ 2 Ret ( = HD 20807
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/21580
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A temperature condensation trend in the debris-disk binary system ζ2 RetSaffe, CarlosFlores Trivigno, Matias GastonJaque Arancibia, Marcelo DanielBuccino, Andrea PaolaJofre, Jorge EmilianoStars: abundancesStars: planetary systemsStars: binariestars: individual: ζ 1 Ret ( = HD 20766), ζ 2 Ret ( = HD 20807https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We explore condensation temperature Tc trends in the unique binary systemZet1 Ret - Zet2 Ret, to determine whether there is a depletion of refractories,which could be related to the planet formation process. The star Zet2 Ret hostsa debris disk which was detected by an IR excess and confirmed by directimaging and numerical simulations, while Zet1 Ret does not present IR excessnor planets. We carried out a high-precision abundance determination in bothcomponents of the binary system via a line-by-line, strictly differentialapproach. The stellar parameters Teff , log g, [Fe/H] and vturb were determinedby imposing differential ionization and excitation equilibrium of Fe I and FeII lines, with an updated version of the program FUNDPAR. The star Zet1 Retresulted slightly more metal rich than Zet2 Ret by 0.02 dex. In thedifferential calculation of Zet1 Ret using Zet2 Ret as reference, theabundances of the refractory elements resulted higher than the volatileelements, and the trend of the refractory elements with Tc showed a positiveslope. These facts together show a lack of refractory elements in Zet2 Ret (adebris-disk host) relative to Zet1 Ret. The Tc trend would be in agreement withthe proposed signature of planet formation (Melendez et al. 2009) rather thanpossible Galactic Chemical Evolution or age effects, which are largelydiminished here. Then, following the interpretation of Melendez et al. (2009),we propose an scenario in which the refractory elements depleted in Zet2 Retare possibly locked-up in the rocky material that orbits this star and producethe debris disk observed around this object. We estimated a lower limit ofMrock = 3 Me for the rocky mass of depleted material, which is compatible witha rough estimation of 3-50 Me of a debris disk mass around a solar-type star.Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geología; ArgentinaFil: Flores Trivigno, Matias Gaston. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Buccino, Andrea Paola. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaEDP Sciences2016-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21580Saffe, Carlos; Flores Trivigno, Matias Gaston; Jaque Arancibia, Marcelo Daniel; Buccino, Andrea Paola; Jofre, Jorge Emiliano; A temperature condensation trend in the debris-disk binary system ζ2 Ret; EDP Sciences; Astronomy and Astrophysics; 588; A81; 2-2016; 1-70004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/04/aa28043-15/aa28043-15.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201528043info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:46:27Zoai:ri.conicet.gov.ar:11336/21580instacron: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 09:46:27.434CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A temperature condensation trend in the debris-disk binary system ζ2 Ret
title A temperature condensation trend in the debris-disk binary system ζ2 Ret
spellingShingle A temperature condensation trend in the debris-disk binary system ζ2 Ret
Saffe, Carlos
Stars: abundances
Stars: planetary systems
Stars: binaries
tars: individual: ζ 1 Ret ( = HD 20766), ζ 2 Ret ( = HD 20807
title_short A temperature condensation trend in the debris-disk binary system ζ2 Ret
title_full A temperature condensation trend in the debris-disk binary system ζ2 Ret
title_fullStr A temperature condensation trend in the debris-disk binary system ζ2 Ret
title_full_unstemmed A temperature condensation trend in the debris-disk binary system ζ2 Ret
title_sort A temperature condensation trend in the debris-disk binary system ζ2 Ret
dc.creator.none.fl_str_mv Saffe, Carlos
Flores Trivigno, Matias Gaston
Jaque Arancibia, Marcelo Daniel
Buccino, Andrea Paola
Jofre, Jorge Emiliano
author Saffe, Carlos
author_facet Saffe, Carlos
Flores Trivigno, Matias Gaston
Jaque Arancibia, Marcelo Daniel
Buccino, Andrea Paola
Jofre, Jorge Emiliano
author_role author
author2 Flores Trivigno, Matias Gaston
Jaque Arancibia, Marcelo Daniel
Buccino, Andrea Paola
Jofre, Jorge Emiliano
author2_role author
author
author
author
dc.subject.none.fl_str_mv Stars: abundances
Stars: planetary systems
Stars: binaries
tars: individual: ζ 1 Ret ( = HD 20766), ζ 2 Ret ( = HD 20807
topic Stars: abundances
Stars: planetary systems
Stars: binaries
tars: individual: ζ 1 Ret ( = HD 20766), ζ 2 Ret ( = HD 20807
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 explore condensation temperature Tc trends in the unique binary systemZet1 Ret - Zet2 Ret, to determine whether there is a depletion of refractories,which could be related to the planet formation process. The star Zet2 Ret hostsa debris disk which was detected by an IR excess and confirmed by directimaging and numerical simulations, while Zet1 Ret does not present IR excessnor planets. We carried out a high-precision abundance determination in bothcomponents of the binary system via a line-by-line, strictly differentialapproach. The stellar parameters Teff , log g, [Fe/H] and vturb were determinedby imposing differential ionization and excitation equilibrium of Fe I and FeII lines, with an updated version of the program FUNDPAR. The star Zet1 Retresulted slightly more metal rich than Zet2 Ret by 0.02 dex. In thedifferential calculation of Zet1 Ret using Zet2 Ret as reference, theabundances of the refractory elements resulted higher than the volatileelements, and the trend of the refractory elements with Tc showed a positiveslope. These facts together show a lack of refractory elements in Zet2 Ret (adebris-disk host) relative to Zet1 Ret. The Tc trend would be in agreement withthe proposed signature of planet formation (Melendez et al. 2009) rather thanpossible Galactic Chemical Evolution or age effects, which are largelydiminished here. Then, following the interpretation of Melendez et al. (2009),we propose an scenario in which the refractory elements depleted in Zet2 Retare possibly locked-up in the rocky material that orbits this star and producethe debris disk observed around this object. We estimated a lower limit ofMrock = 3 Me for the rocky mass of depleted material, which is compatible witha rough estimation of 3-50 Me of a debris disk mass around a solar-type star.
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geología; Argentina
Fil: Flores Trivigno, Matias Gaston. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Jaque Arancibia, Marcelo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Buccino, Andrea Paola. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
Fil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
description We explore condensation temperature Tc trends in the unique binary systemZet1 Ret - Zet2 Ret, to determine whether there is a depletion of refractories,which could be related to the planet formation process. The star Zet2 Ret hostsa debris disk which was detected by an IR excess and confirmed by directimaging and numerical simulations, while Zet1 Ret does not present IR excessnor planets. We carried out a high-precision abundance determination in bothcomponents of the binary system via a line-by-line, strictly differentialapproach. The stellar parameters Teff , log g, [Fe/H] and vturb were determinedby imposing differential ionization and excitation equilibrium of Fe I and FeII lines, with an updated version of the program FUNDPAR. The star Zet1 Retresulted slightly more metal rich than Zet2 Ret by 0.02 dex. In thedifferential calculation of Zet1 Ret using Zet2 Ret as reference, theabundances of the refractory elements resulted higher than the volatileelements, and the trend of the refractory elements with Tc showed a positiveslope. These facts together show a lack of refractory elements in Zet2 Ret (adebris-disk host) relative to Zet1 Ret. The Tc trend would be in agreement withthe proposed signature of planet formation (Melendez et al. 2009) rather thanpossible Galactic Chemical Evolution or age effects, which are largelydiminished here. Then, following the interpretation of Melendez et al. (2009),we propose an scenario in which the refractory elements depleted in Zet2 Retare possibly locked-up in the rocky material that orbits this star and producethe debris disk observed around this object. We estimated a lower limit ofMrock = 3 Me for the rocky mass of depleted material, which is compatible witha rough estimation of 3-50 Me of a debris disk mass around a solar-type star.
publishDate 2016
dc.date.none.fl_str_mv 2016-02
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/11336/21580
Saffe, Carlos; Flores Trivigno, Matias Gaston; Jaque Arancibia, Marcelo Daniel; Buccino, Andrea Paola; Jofre, Jorge Emiliano; A temperature condensation trend in the debris-disk binary system ζ2 Ret; EDP Sciences; Astronomy and Astrophysics; 588; A81; 2-2016; 1-7
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/21580
identifier_str_mv Saffe, Carlos; Flores Trivigno, Matias Gaston; Jaque Arancibia, Marcelo Daniel; Buccino, Andrea Paola; Jofre, Jorge Emiliano; A temperature condensation trend in the debris-disk binary system ζ2 Ret; EDP Sciences; Astronomy and Astrophysics; 588; A81; 2-2016; 1-7
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/2016/04/aa28043-15/aa28043-15.html
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201528043
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
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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score 13.070432

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