A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry
- Autores
- Corti, Mariela Alejandra; Orellana, Rosa Beatriz; Bosch, Guillermo Luis
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrometric and spectrophotometric analyses, and estimate its distance and evolutionary stage. Methods. We used our own visual spectroscopic and UBV photometric data of a 300 × 300 region centered at a = 8h44m47:2s, δ =-45°58055.500. This information enabled us to estimate the spectral classification and distance of all stars present in the region. The proper motion was analyzed with data of the UCAC 5 catalog and was used to identify the members of this association. We added JHK data from 2MASS and IRAS catalogs to check for the presence of infrared (IR) excess stars. Results. We found that Bochum 7 is an OB association with at least 27 identified stellar members (l = 265.12, b =-2) at a distance of '5640 pc. Its proper motion is μacosd =-4:92 ± 0:08 mas yr-1, μd = 3:26 ± 0:08 mas yr-1. We derived an average heliocentric radial velocity of ∼35 km s-1 and were able to confirm the binary nature of the (ALS 1135) system and detect four new binary star candidates. Analysis of data for massive Bo 7 star candidates points towards a young age (=3 × 106 years old) for the association, although the presence of a previous episode of star formation remains to be analyzed.
Fil: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Orellana, Rosa Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Bosch, Guillermo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina - Materia
-
Catalogs
Open Clusters And Associations: Individual: Bochum 7
Proper Motions
Stars: Early-Type - 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:11336/82403
Ver los metadatos del registro completo
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CONICET Digital (CONICET) |
spelling |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometryCorti, Mariela AlejandraOrellana, Rosa BeatrizBosch, Guillermo LuisCatalogsOpen Clusters And Associations: Individual: Bochum 7Proper MotionsStars: Early-Typehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrometric and spectrophotometric analyses, and estimate its distance and evolutionary stage. Methods. We used our own visual spectroscopic and UBV photometric data of a 300 × 300 region centered at a = 8h44m47:2s, δ =-45°58055.500. This information enabled us to estimate the spectral classification and distance of all stars present in the region. The proper motion was analyzed with data of the UCAC 5 catalog and was used to identify the members of this association. We added JHK data from 2MASS and IRAS catalogs to check for the presence of infrared (IR) excess stars. Results. We found that Bochum 7 is an OB association with at least 27 identified stellar members (l = 265.12, b =-2) at a distance of '5640 pc. Its proper motion is μacosd =-4:92 ± 0:08 mas yr-1, μd = 3:26 ± 0:08 mas yr-1. We derived an average heliocentric radial velocity of ∼35 km s-1 and were able to confirm the binary nature of the (ALS 1135) system and detect four new binary star candidates. Analysis of data for massive Bo 7 star candidates points towards a young age (=3 × 106 years old) for the association, although the presence of a previous episode of star formation remains to be analyzed.Fil: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Orellana, Rosa Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Bosch, Guillermo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaEDP Sciences2018-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/82403Corti, Mariela Alejandra; Orellana, Rosa Beatriz; Bosch, Guillermo Luis; A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry; EDP Sciences; Astronomy and Astrophysics; 616; A40; 8-2018; 1-100004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201731661info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2018/08/aa31661-17/aa31661-17.htmlinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1804.10672info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:45:58Zoai:ri.conicet.gov.ar:11336/82403instacron: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 10:45:58.934CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
title |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
spellingShingle |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry Corti, Mariela Alejandra Catalogs Open Clusters And Associations: Individual: Bochum 7 Proper Motions Stars: Early-Type |
title_short |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
title_full |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
title_fullStr |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
title_full_unstemmed |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
title_sort |
A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry |
dc.creator.none.fl_str_mv |
Corti, Mariela Alejandra Orellana, Rosa Beatriz Bosch, Guillermo Luis |
author |
Corti, Mariela Alejandra |
author_facet |
Corti, Mariela Alejandra Orellana, Rosa Beatriz Bosch, Guillermo Luis |
author_role |
author |
author2 |
Orellana, Rosa Beatriz Bosch, Guillermo Luis |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Catalogs Open Clusters And Associations: Individual: Bochum 7 Proper Motions Stars: Early-Type |
topic |
Catalogs Open Clusters And Associations: Individual: Bochum 7 Proper Motions Stars: Early-Type |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrometric and spectrophotometric analyses, and estimate its distance and evolutionary stage. Methods. We used our own visual spectroscopic and UBV photometric data of a 300 × 300 region centered at a = 8h44m47:2s, δ =-45°58055.500. This information enabled us to estimate the spectral classification and distance of all stars present in the region. The proper motion was analyzed with data of the UCAC 5 catalog and was used to identify the members of this association. We added JHK data from 2MASS and IRAS catalogs to check for the presence of infrared (IR) excess stars. Results. We found that Bochum 7 is an OB association with at least 27 identified stellar members (l = 265.12, b =-2) at a distance of '5640 pc. Its proper motion is μacosd =-4:92 ± 0:08 mas yr-1, μd = 3:26 ± 0:08 mas yr-1. We derived an average heliocentric radial velocity of ∼35 km s-1 and were able to confirm the binary nature of the (ALS 1135) system and detect four new binary star candidates. Analysis of data for massive Bo 7 star candidates points towards a young age (=3 × 106 years old) for the association, although the presence of a previous episode of star formation remains to be analyzed. Fil: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Orellana, Rosa Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Bosch, Guillermo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina |
description |
Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrometric and spectrophotometric analyses, and estimate its distance and evolutionary stage. Methods. We used our own visual spectroscopic and UBV photometric data of a 300 × 300 region centered at a = 8h44m47:2s, δ =-45°58055.500. This information enabled us to estimate the spectral classification and distance of all stars present in the region. The proper motion was analyzed with data of the UCAC 5 catalog and was used to identify the members of this association. We added JHK data from 2MASS and IRAS catalogs to check for the presence of infrared (IR) excess stars. Results. We found that Bochum 7 is an OB association with at least 27 identified stellar members (l = 265.12, b =-2) at a distance of '5640 pc. Its proper motion is μacosd =-4:92 ± 0:08 mas yr-1, μd = 3:26 ± 0:08 mas yr-1. We derived an average heliocentric radial velocity of ∼35 km s-1 and were able to confirm the binary nature of the (ALS 1135) system and detect four new binary star candidates. Analysis of data for massive Bo 7 star candidates points towards a young age (=3 × 106 years old) for the association, although the presence of a previous episode of star formation remains to be analyzed. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-08 |
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/11336/82403 Corti, Mariela Alejandra; Orellana, Rosa Beatriz; Bosch, Guillermo Luis; A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry; EDP Sciences; Astronomy and Astrophysics; 616; A40; 8-2018; 1-10 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/82403 |
identifier_str_mv |
Corti, Mariela Alejandra; Orellana, Rosa Beatriz; Bosch, Guillermo Luis; A search for OB stars in the field of the galactic OB association Bochum 7: II. Proper motion and IR photometry; EDP Sciences; Astronomy and Astrophysics; 616; A40; 8-2018; 1-10 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/doi/10.1051/0004-6361/201731661 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2018/08/aa31661-17/aa31661-17.html info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1804.10672 |
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 |
dc.publisher.none.fl_str_mv |
EDP Sciences |
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EDP Sciences |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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