Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope

Context. Many massive stars have nearby companions whose presence hamper their characterization through spectroscopy. Aims. We want to obtain spatially resolved spectroscopy of close massive visual binaries to derive their spectral types. Methods. We obtained a large number of short long-slit spectr...

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Autores: Maíz Apellániz, J., Barbá, R. H., Simón Díaz, S., Sota, A., Trigueros Páez, E., Caballero, J. A., Alfaro, Emilio J.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2018
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:20.500.12666/737
Acceso en línea:https://www.aanda.org/articles/aa/abs/2018/07/aa32885-18/aa32885-18.html
http://hdl.handle.net/20.500.12666/737
Access Level:acceso abierto
Palabra clave:Binaries: spectroscopic
Binaries: visual
Methods: data analysis
Stars: early type
Stars: massive
Techniques: spectroscopic
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network_name_str España
repository_id_str
dc.title.none.fl_str_mv Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
title Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
spellingShingle Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
Maíz Apellániz, J.
Binaries: spectroscopic
Binaries: visual
Methods: data analysis
Stars: early type
Stars: massive
Techniques: spectroscopic
title_short Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
title_full Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
title_fullStr Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
title_full_unstemmed Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
title_sort Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
dc.creator.none.fl_str_mv Maíz Apellániz, J.
Barbá, R. H.
Simón Díaz, S.
Sota, A.
Trigueros Páez, E.
Caballero, J. A.
Alfaro, Emilio J.
author Maíz Apellániz, J.
author_facet Maíz Apellániz, J.
Barbá, R. H.
Simón Díaz, S.
Sota, A.
Trigueros Páez, E.
Caballero, J. A.
Alfaro, Emilio J.
author_role author
author2 Barbá, R. H.
Simón Díaz, S.
Sota, A.
Trigueros Páez, E.
Caballero, J. A.
Alfaro, Emilio J.
author2_role author
author
author
author
author
author
dc.contributor.none.fl_str_mv Maíz Apellániz, J. [0000-0003-0825-3443]
Barbá, R. H. [0000-0003-1086-1579]
Simón Díaz, S. [0000-0003-1168-3524]
Trigueros Páez, E. [0000-0001-6770-1977]
Ministerio de Economía y Competitividad (MINECO)
Agencia Estatal de Investigación (AEI)
dc.subject.none.fl_str_mv Binaries: spectroscopic
Binaries: visual
Methods: data analysis
Stars: early type
Stars: massive
Techniques: spectroscopic
topic Binaries: spectroscopic
Binaries: visual
Methods: data analysis
Stars: early type
Stars: massive
Techniques: spectroscopic
description Context. Many massive stars have nearby companions whose presence hamper their characterization through spectroscopy. Aims. We want to obtain spatially resolved spectroscopy of close massive visual binaries to derive their spectral types. Methods. We obtained a large number of short long-slit spectroscopic exposures of five close binaries under good seeing conditions. We selected those with the best characteristics, extracted the spectra using multiple-profile fitting, and combined the results to derive spatially separated spectra. Results. We demonstrate the usefulness of Lucky Spectroscopy by presenting the spatially resolved spectra of the components of each system, in two cases with separations of only ~0.′′3. Those are δ Ori Aa+Ab (resolved in the optical for the first time) and σ Ori AaAb+B (first time ever resolved). We also spatially resolve 15 Mon AaAb+B, ζ Ori AaAb+B (both previously resolved with GOSSS, the Galactic O-Star Spectroscopic Survey), and η Ori AaAb+B, a system with two spectroscopic B+B binaries and a fifth visual component. The systems have in common that they are composed of an inner pair of slow rotators orbited by one or more fast rotators, a characteristic that could have consequences for the theories of massive star formation.
publishDate 2018
dc.date.none.fl_str_mv 2018
2022
2022
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://www.aanda.org/articles/aa/abs/2018/07/aa32885-18/aa32885-18.html
http://hdl.handle.net/20.500.12666/737
url https://www.aanda.org/articles/aa/abs/2018/07/aa32885-18/aa32885-18.html
http://hdl.handle.net/20.500.12666/737
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv ENANAS MARRONES Y PLANETAS AISLADOS Y COMO COMPAÑEROS DE ESTRELLAS
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-1-P
ESTRELLAS MASIVAS EN EL UNIVERSO LOCAL
CARTOGRAFIANDO EL CIELO: SONDEOS EN EL OPTICO E INFRARROJO DE LA VIA LACTEA II
STRELLAS DE GRAN MASA COMO PROGENITORES DE SUPERNOVAS
CARTOGRAFIANDO EL CIELO: SONDEOS DE ESTRELLAS O DE LA VIA LACTEA
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-2-P
info:eu-repo/grantAgreement/MINECO//AYA2015-68012-C2-1-P
info:eu-repo/grantAgreement/MINECO//AYA2015-68012-C2-2-P
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-79425-C3-2-P
dc.rights.none.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
© ESO 2018
https://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
© ESO 2018
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 EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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
repository.name.fl_str_mv
repository.mail.fl_str_mv
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spelling Lucky Spectroscopy, an equivalent technique to Lucky Imaging Spatially resolved spectroscopy of massive close visual binaries using the William Herschel TelescopeMaíz Apellániz, J.Barbá, R. H.Simón Díaz, S.Sota, A.Trigueros Páez, E.Caballero, J. A.Alfaro, Emilio J. Binaries: spectroscopicBinaries: visualMethods: data analysisStars: early typeStars: massiveTechniques: spectroscopicContext. Many massive stars have nearby companions whose presence hamper their characterization through spectroscopy. Aims. We want to obtain spatially resolved spectroscopy of close massive visual binaries to derive their spectral types. Methods. We obtained a large number of short long-slit spectroscopic exposures of five close binaries under good seeing conditions. We selected those with the best characteristics, extracted the spectra using multiple-profile fitting, and combined the results to derive spatially separated spectra. Results. We demonstrate the usefulness of Lucky Spectroscopy by presenting the spatially resolved spectra of the components of each system, in two cases with separations of only ~0.′′3. Those are δ Ori Aa+Ab (resolved in the optical for the first time) and σ Ori AaAb+B (first time ever resolved). We also spatially resolve 15 Mon AaAb+B, ζ Ori AaAb+B (both previously resolved with GOSSS, the Galactic O-Star Spectroscopic Survey), and η Ori AaAb+B, a system with two spectroscopic B+B binaries and a fifth visual component. The systems have in common that they are composed of an inner pair of slow rotators orbited by one or more fast rotators, a characteristic that could have consequences for the theories of massive star formation.As we were about to submit this paper, we received the sad news of the death of Nolan R. Walborn after a long battle with cancer. As he was the inspiration for GOSSS, we would like to dedicate this paper to him. May he rest in peace. This work has made use of the Washington Double Star Catalog (Mason et al. 2001). The authors would like to thank the personnel of the Isaac Newton Group of telescopes for their support throughout the years, with a special mention to Cecilia Fariña for her help with the setup for Lucky Spectroscopy. The first author is amazed that the instrument he used for his PhD Thesis is still working one quarter of a century later and is not yet surpassed in some of its characteristics. We acknowledge support from the Spanish Government Ministerio de Economía y Competitividad (MINECO) through grants AYA2016-75 931-C2-1/2-P (J.M.A., A.S., E.T.P., and E.J.A), AYA2015-68 012-C2-1/2-P (S.S.-D. and E.T.P.) and AYA2016-79 425-C3-2-P (J.A.C.). R.H.B. acknowledges support from the ESAC Faculty Council Visitor Program.PeerreviewEDP SciencesMaíz Apellániz, J. [0000-0003-0825-3443]Barbá, R. H. [0000-0003-1086-1579]Simón Díaz, S. [0000-0003-1168-3524]Trigueros Páez, E. [0000-0001-6770-1977]Ministerio de Economía y Competitividad (MINECO)Agencia Estatal de Investigación (AEI)202220222018info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://www.aanda.org/articles/aa/abs/2018/07/aa32885-18/aa32885-18.htmlhttp://hdl.handle.net/20.500.12666/737reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)InglésENANAS MARRONES Y PLANETAS AISLADOS Y COMO COMPAÑEROS DE ESTRELLASinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-1-PESTRELLAS MASIVAS EN EL UNIVERSO LOCALCARTOGRAFIANDO EL CIELO: SONDEOS EN EL OPTICO E INFRARROJO DE LA VIA LACTEA IISTRELLAS DE GRAN MASA COMO PROGENITORES DE SUPERNOVASCARTOGRAFIANDO EL CIELO: SONDEOS DE ESTRELLAS O DE LA VIA LACTEAinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-2-Pinfo:eu-repo/grantAgreement/MINECO//AYA2015-68012-C2-1-Pinfo:eu-repo/grantAgreement/MINECO//AYA2015-68012-C2-2-Pinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-79425-C3-2-PAttribution-NonCommercial-NoDerivatives 4.0 International© ESO 2018https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/7372026-06-23T12:46:37Z
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