The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf

We present 10 new ultracool dwarfs in seven wide binary systems discovered using Gaia second data release data, identified as part of our Gaia Ultra-Cool Dwarf Sample project. The seven systems presented here include an L1 companion to the G5 IV star HD 164507, an L1: companion to the V478 Lyr AB sy...

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Autores: Marocco, F., Smart, R. L., Mamajek, E. E., Sarro, L. M., Burgasser, A. J., Caballero, J. A., Rees, J. M., Caselden, D., Cruz, K. L., Van Linge, R., Pinfield, David J.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:España
Institución:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/300
Acceso en línea:https://academic.oup.com/mnras/article/494/4/4891/5820239
http://hdl.handle.net/20.500.12666/300
Access Level:acceso abierto
Palabra clave:Binaries: visual
Brown dwarfs
Stars: individual: HD 164507
V478 Lyr
CD-28 8692
LT UMa
Stars: low-mass
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spelling The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarfMarocco, F.Smart, R. L.Mamajek, E. E.Sarro, L. M.Burgasser, A. J.Caballero, J. A.Rees, J. M.Caselden, D.Cruz, K. L.Van Linge, R.Pinfield, David J.Binaries: visualBrown dwarfsStars: individual: HD 164507V478 LyrCD-28 8692LT UMaStars: low-massWe present 10 new ultracool dwarfs in seven wide binary systems discovered using Gaia second data release data, identified as part of our Gaia Ultra-Cool Dwarf Sample project. The seven systems presented here include an L1 companion to the G5 IV star HD 164507, an L1: companion to the V478 Lyr AB system, an L2 companion to the metal-poor K5 V star CD-28 8692, an M9 V companion to the young variable K0 V star LT UMa, and three low-mass binaries consisting of late Ms and early Ls. The HD 164507, CD-28 8692, V478 Lyr, and LT UMa systems are particularly important benchmarks, because the primaries are well characterized and offer excellent constraints on the atmospheric parameters and ages of the companions. We find that the M8 V star 2MASS J23253550+4608163 is ∼2.5 mag overluminous compared to M dwarfs of similar spectral type, but at the same time it does not exhibit obvious peculiarities in its near-infrared spectrum. Its overluminosity cannot be explained by unresolved binarity alone. Finally, we present an L1+L2 system with a projected physical separation of 959 au, making this the widest L + L binary currently known.FM acknowledges support by the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Universities Space Research Association under a contract with NASA. SPLAT is a collaborative project of research students in UCSD Cool Star Lab. Contributors to SPLAT have included Christian Aganze, Jessica Birky, Daniella Bardalez Gagliuffi, Adam Burgasser (PI), Caleb Choban, Andrew Davis, Ivanna Escala, Aishwarya Iyer, Yuhui Jin, Mike Lopez, Alex Mendez, Gretel Mercado, Elizabeth Moreno Hilario, Johnny Parra, Maitrayee Sahi, Adrian Suarez, Melisa Tallis, Tomoki Tamiya, Chris Theissen and Russell van Linge. This project is supported by the National Aeronautics and Space Administration under grant no. NNX15AI75G. This publication makes use of VOSA, developed under the Spanish Virtual Observatory project supported by the Spanish MINECO through grant AyA2017-84089; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).Peer reviewOxford Academics: Oxford University PressUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-07370000-0002-5622-51910000-0002-4424-47660000-0002-6523-9536National Aeronautics and Space Administration (NASA)Agencia Estatal de Investigación (AEI)202120212020info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://academic.oup.com/mnras/article/494/4/4891/5820239http://hdl.handle.net/20.500.12666/300reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)InglésEL OBSERVATORIO VIRTUAL ESPAÑOL. EXPLOTACION CIENTIFICO-TECNICA DE ARCHIVOS ASTRONOMICOSinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84089-PAttribution-NonCommercial-NoDerivatives 4.0 InternationalCopyright © 2020, Oxford University Presshttps://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/3002026-06-23T12:46:37Z
dc.title.none.fl_str_mv The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
title The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
spellingShingle The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
Marocco, F.
Binaries: visual
Brown dwarfs
Stars: individual: HD 164507
V478 Lyr
CD-28 8692
LT UMa
Stars: low-mass
title_short The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
title_full The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
title_fullStr The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
title_full_unstemmed The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
title_sort The Gaia Ultra-Cool Dwarf Sample – III: seven new multiple systems containing at least one Gaia DR2 ultracool dwarf
dc.creator.none.fl_str_mv Marocco, F.
Smart, R. L.
Mamajek, E. E.
Sarro, L. M.
Burgasser, A. J.
Caballero, J. A.
Rees, J. M.
Caselden, D.
Cruz, K. L.
Van Linge, R.
Pinfield, David J.
author Marocco, F.
author_facet Marocco, F.
Smart, R. L.
Mamajek, E. E.
Sarro, L. M.
Burgasser, A. J.
Caballero, J. A.
Rees, J. M.
Caselden, D.
Cruz, K. L.
Van Linge, R.
Pinfield, David J.
author_role author
author2 Smart, R. L.
Mamajek, E. E.
Sarro, L. M.
Burgasser, A. J.
Caballero, J. A.
Rees, J. M.
Caselden, D.
Cruz, K. L.
Van Linge, R.
Pinfield, David J.
author2_role author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
0000-0002-5622-5191
0000-0002-4424-4766
0000-0002-6523-9536
National Aeronautics and Space Administration (NASA)
Agencia Estatal de Investigación (AEI)
dc.subject.none.fl_str_mv Binaries: visual
Brown dwarfs
Stars: individual: HD 164507
V478 Lyr
CD-28 8692
LT UMa
Stars: low-mass
topic Binaries: visual
Brown dwarfs
Stars: individual: HD 164507
V478 Lyr
CD-28 8692
LT UMa
Stars: low-mass
description We present 10 new ultracool dwarfs in seven wide binary systems discovered using Gaia second data release data, identified as part of our Gaia Ultra-Cool Dwarf Sample project. The seven systems presented here include an L1 companion to the G5 IV star HD 164507, an L1: companion to the V478 Lyr AB system, an L2 companion to the metal-poor K5 V star CD-28 8692, an M9 V companion to the young variable K0 V star LT UMa, and three low-mass binaries consisting of late Ms and early Ls. The HD 164507, CD-28 8692, V478 Lyr, and LT UMa systems are particularly important benchmarks, because the primaries are well characterized and offer excellent constraints on the atmospheric parameters and ages of the companions. We find that the M8 V star 2MASS J23253550+4608163 is ∼2.5 mag overluminous compared to M dwarfs of similar spectral type, but at the same time it does not exhibit obvious peculiarities in its near-infrared spectrum. Its overluminosity cannot be explained by unresolved binarity alone. Finally, we present an L1+L2 system with a projected physical separation of 959 au, making this the widest L + L binary currently known.
publishDate 2020
dc.date.none.fl_str_mv 2020
2021
2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://academic.oup.com/mnras/article/494/4/4891/5820239
http://hdl.handle.net/20.500.12666/300
url https://academic.oup.com/mnras/article/494/4/4891/5820239
http://hdl.handle.net/20.500.12666/300
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv EL OBSERVATORIO VIRTUAL ESPAÑOL. EXPLOTACION CIENTIFICO-TECNICA DE ARCHIVOS ASTRONOMICOS
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84089-P
dc.rights.none.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Copyright © 2020, Oxford University Press
https://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Copyright © 2020, Oxford University Press
https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Oxford Academics: Oxford University Press
publisher.none.fl_str_mv Oxford Academics: Oxford University Press
dc.source.none.fl_str_mv reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname:Instituto Nacional de Técnica Aeroespacial (INTA)
instname_str Instituto Nacional de Técnica Aeroespacial (INTA)
reponame_str DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
collection DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
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repository.mail.fl_str_mv
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