Gamma-rays from the compact colliding wind region in Cyg OB2 #5
- Autores
- Araudo, Anabella Teresa; Ortiz Leon, Gisella; Rodríguez, Luis Felipe
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact (and recently detected) collidingwind region in the multiple stellar system Cyg OB2 #5. We focus ourstudy on the detectability of the produced γ-rays.
Fil: Araudo, Anabella Teresa. 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
Fil: Ortiz Leon, Gisella. Universidad Nacional Autónoma de México; México
Fil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; México
High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy
Heidelberg
Alemania
Max-Planck-Institut für Kernphysik - Materia
-
STARS: BINARIES
STARS: INDIVIDUAL; CYG OB2 5
RADIATION MECHANISMS: NON THERMAL
GAMMA RAYS: THEORY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/152650
Ver los metadatos del registro completo
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Gamma-rays from the compact colliding wind region in Cyg OB2 #5Araudo, Anabella TeresaOrtiz Leon, GisellaRodríguez, Luis FelipeSTARS: BINARIESSTARS: INDIVIDUAL; CYG OB2 5RADIATION MECHANISMS: NON THERMALGAMMA RAYS: THEORYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact (and recently detected) collidingwind region in the multiple stellar system Cyg OB2 #5. We focus ourstudy on the detectability of the produced γ-rays.Fil: Araudo, Anabella Teresa. 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; ArgentinaFil: Ortiz Leon, Gisella. Universidad Nacional Autónoma de México; MéxicoFil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; MéxicoHigh Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray AstronomyHeidelbergAlemaniaMax-Planck-Institut für KernphysikAmerican Institute of PhysicsAharonian, Felix A.Hofmann, WernerRieger, Frank M.2012info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/152650Gamma-rays from the compact colliding wind region in Cyg OB2 #5; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 422-4259780735411234CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4772287info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4772287Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-12T09:54:08Zoai:ri.conicet.gov.ar:11336/152650instacron: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:34982025-11-12 09:54:08.759CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| title |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| spellingShingle |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 Araudo, Anabella Teresa STARS: BINARIES STARS: INDIVIDUAL; CYG OB2 5 RADIATION MECHANISMS: NON THERMAL GAMMA RAYS: THEORY |
| title_short |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| title_full |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| title_fullStr |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| title_full_unstemmed |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| title_sort |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5 |
| dc.creator.none.fl_str_mv |
Araudo, Anabella Teresa Ortiz Leon, Gisella Rodríguez, Luis Felipe |
| author |
Araudo, Anabella Teresa |
| author_facet |
Araudo, Anabella Teresa Ortiz Leon, Gisella Rodríguez, Luis Felipe |
| author_role |
author |
| author2 |
Ortiz Leon, Gisella Rodríguez, Luis Felipe |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
Aharonian, Felix A. Hofmann, Werner Rieger, Frank M. |
| dc.subject.none.fl_str_mv |
STARS: BINARIES STARS: INDIVIDUAL; CYG OB2 5 RADIATION MECHANISMS: NON THERMAL GAMMA RAYS: THEORY |
| topic |
STARS: BINARIES STARS: INDIVIDUAL; CYG OB2 5 RADIATION MECHANISMS: NON THERMAL GAMMA RAYS: THEORY |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact (and recently detected) collidingwind region in the multiple stellar system Cyg OB2 #5. We focus ourstudy on the detectability of the produced γ-rays. Fil: Araudo, Anabella Teresa. 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 Fil: Ortiz Leon, Gisella. Universidad Nacional Autónoma de México; México Fil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; México High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy Heidelberg Alemania Max-Planck-Institut für Kernphysik |
| description |
In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact (and recently detected) collidingwind region in the multiple stellar system Cyg OB2 #5. We focus ourstudy on the detectability of the produced γ-rays. |
| publishDate |
2012 |
| dc.date.none.fl_str_mv |
2012 |
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info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Reunión Book http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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publishedVersion |
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http://hdl.handle.net/11336/152650 Gamma-rays from the compact colliding wind region in Cyg OB2 #5; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 422-425 9780735411234 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/152650 |
| identifier_str_mv |
Gamma-rays from the compact colliding wind region in Cyg OB2 #5; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 422-425 9780735411234 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4772287 info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4772287 |
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openAccess |
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Internacional |
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American Institute of Physics |
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American Institute of Physics |
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