Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22)
- Autores
- Combi, Jorge Ariel
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- We report preliminary results of a multi-wavelength (radio-optical-X-ray) study of the massive star CPD -59 2629 (Tr 16-22) in the Carina Nebula (NGC 3372). This star has historically shown a large X-ray excess (log L_{X}/L_{bol} < -6 or even larger), which is one order of magnitude larger than expected from single massive O-type stars. A colliding wind scenario is a plausible explanation. On this subject, we searched for non-thermal radio emission and used high-resolution optical spectroscopy to check for multiplicity and investigate the nature of the stars as well as the origin and excess of the X-ray emission. We detected long-term radial-velocity and X-ray variability. Both results suggest that Tr 16-22 is a long-term massive binary system and a variable colliding wind shock scenario.
Fil: Combi, Jorge Ariel. 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
39th Liège Astrophysical Colloquium
Liège
Bélgica
Société Royale des Sciences de Liège - Materia
-
STARS
X-RAY EMISSION
OPTICAL OBSERVATIONS - 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:11336/226618
Ver los metadatos del registro completo
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Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22)Combi, Jorge ArielSTARSX-RAY EMISSIONOPTICAL OBSERVATIONShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report preliminary results of a multi-wavelength (radio-optical-X-ray) study of the massive star CPD -59 2629 (Tr 16-22) in the Carina Nebula (NGC 3372). This star has historically shown a large X-ray excess (log L_{X}/L_{bol} < -6 or even larger), which is one order of magnitude larger than expected from single massive O-type stars. A colliding wind scenario is a plausible explanation. On this subject, we searched for non-thermal radio emission and used high-resolution optical spectroscopy to check for multiplicity and investigate the nature of the stars as well as the origin and excess of the X-ray emission. We detected long-term radial-velocity and X-ray variability. Both results suggest that Tr 16-22 is a long-term massive binary system and a variable colliding wind shock scenario.Fil: Combi, Jorge Ariel. 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; Argentina39th Liège Astrophysical ColloquiumLiègeBélgicaSociété Royale des Sciences de LiègeSociété Royale des Sciences de LiègeRauw, G.De Becker, M.Nazé, Y.Vreux, J.-M.William, P.2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/226618Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22); 39th Liège Astrophysical Colloquium; Liège; Bélgica; 2010; 644-6471783-5720CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://articles.adsabs.harvard.edu/full/2011BSRSL..80..644Cinfo:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2011BSRSL..80..644C/abstractInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:24Zoai:ri.conicet.gov.ar:11336/226618instacron: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 10:04:25.011CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
title |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
spellingShingle |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) Combi, Jorge Ariel STARS X-RAY EMISSION OPTICAL OBSERVATIONS |
title_short |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
title_full |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
title_fullStr |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
title_full_unstemmed |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
title_sort |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22) |
dc.creator.none.fl_str_mv |
Combi, Jorge Ariel |
author |
Combi, Jorge Ariel |
author_facet |
Combi, Jorge Ariel |
author_role |
author |
dc.contributor.none.fl_str_mv |
Rauw, G. De Becker, M. Nazé, Y. Vreux, J.-M. William, P. |
dc.subject.none.fl_str_mv |
STARS X-RAY EMISSION OPTICAL OBSERVATIONS |
topic |
STARS X-RAY EMISSION OPTICAL OBSERVATIONS |
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 report preliminary results of a multi-wavelength (radio-optical-X-ray) study of the massive star CPD -59 2629 (Tr 16-22) in the Carina Nebula (NGC 3372). This star has historically shown a large X-ray excess (log L_{X}/L_{bol} < -6 or even larger), which is one order of magnitude larger than expected from single massive O-type stars. A colliding wind scenario is a plausible explanation. On this subject, we searched for non-thermal radio emission and used high-resolution optical spectroscopy to check for multiplicity and investigate the nature of the stars as well as the origin and excess of the X-ray emission. We detected long-term radial-velocity and X-ray variability. Both results suggest that Tr 16-22 is a long-term massive binary system and a variable colliding wind shock scenario. Fil: Combi, Jorge Ariel. 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 39th Liège Astrophysical Colloquium Liège Bélgica Société Royale des Sciences de Liège |
description |
We report preliminary results of a multi-wavelength (radio-optical-X-ray) study of the massive star CPD -59 2629 (Tr 16-22) in the Carina Nebula (NGC 3372). This star has historically shown a large X-ray excess (log L_{X}/L_{bol} < -6 or even larger), which is one order of magnitude larger than expected from single massive O-type stars. A colliding wind scenario is a plausible explanation. On this subject, we searched for non-thermal radio emission and used high-resolution optical spectroscopy to check for multiplicity and investigate the nature of the stars as well as the origin and excess of the X-ray emission. We detected long-term radial-velocity and X-ray variability. Both results suggest that Tr 16-22 is a long-term massive binary system and a variable colliding wind shock scenario. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Congreso Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
status_str |
publishedVersion |
format |
conferenceObject |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/226618 Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22); 39th Liège Astrophysical Colloquium; Liège; Bélgica; 2010; 644-647 1783-5720 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/226618 |
identifier_str_mv |
Multiwavelength study of the intriguing massive star CPD--59 2629 (Tr 16-22); 39th Liège Astrophysical Colloquium; Liège; Bélgica; 2010; 644-647 1783-5720 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://articles.adsabs.harvard.edu/full/2011BSRSL..80..644C info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2011BSRSL..80..644C/abstract |
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 |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
dc.coverage.none.fl_str_mv |
Internacional |
dc.publisher.none.fl_str_mv |
Société Royale des Sciences de Liège |
publisher.none.fl_str_mv |
Société Royale des Sciences de Liège |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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