On the nature of the episodic gamma-ray flare observed in Cygnus X-1
- Autores
- Valle, María Victoria del; Romero, Gustavo Esteban; Orellana, Mariana Dominga
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The high-mass microquasar Cygnus X-1, the best established candidate for a stellar-mass black hole, has been detected in a flaring state at very high energies, E > 200 GeV (Albert et al. 2007). The observation was per- formed by the Atmospheric Cherenkov Telescope MAGIC. It is the first experimental evidence of very high energy emission produced by a galactic stellar-mass black hole. The observed high energy excess occurred in coin- cidence with an X-ray flare. The flare took place at orbital phase = 0.91, being = 1 the moment when the black hole is behind the companion star. In this configuration the absorption of gamma-ray photons produced by photon-photon annihilation with the stellar field is expected to be the highest. We present detailed calculations of the gamma-ray opacity due to pair creation along the whole orbit, and for different locations of the emitter (height above the compact object). We discuss the location of the gamma- ray producing region in Cygnus X-1 and the energetics required to produce the flare.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Física
Ciencias Astronómicas
X ray binaries
Gamma rays
Microquásars
Cygnus X-1 (microcuásar) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/99098
Ver los metadatos del registro completo
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On the nature of the episodic gamma-ray flare observed in Cygnus X-1Valle, María Victoria delRomero, Gustavo EstebanOrellana, Mariana DomingaFísicaCiencias AstronómicasX ray binariesGamma raysMicroquásarsCygnus X-1 (microcuásar)The high-mass microquasar Cygnus X-1, the best established candidate for a stellar-mass black hole, has been detected in a flaring state at very high energies, E > 200 GeV (Albert et al. 2007). The observation was per- formed by the Atmospheric Cherenkov Telescope MAGIC. It is the first experimental evidence of very high energy emission produced by a galactic stellar-mass black hole. The observed high energy excess occurred in coin- cidence with an X-ray flare. The flare took place at orbital phase = 0.91, being = 1 the moment when the black hole is behind the companion star. In this configuration the absorption of gamma-ray photons produced by photon-photon annihilation with the stellar field is expected to be the highest. We present detailed calculations of the gamma-ray opacity due to pair creation along the whole orbit, and for different locations of the emitter (height above the compact object). We discuss the location of the gamma- ray producing region in Cygnus X-1 and the energetics required to produce the flare.Facultad de Ciencias Astronómicas y Geofísicas2009-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf259-262http://sedici.unlp.edu.ar/handle/10915/99098enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/23361info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2009BAAA...52..259Dinfo:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/b52/2009BAAA...52..259D.pdfinfo:eu-repo/semantics/altIdentifier/issn/1669-9521info:eu-repo/semantics/altIdentifier/hdl/11336/23361info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:19:56Zoai:sedici.unlp.edu.ar:10915/99098Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:19:57.151SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
title |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
spellingShingle |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 Valle, María Victoria del Física Ciencias Astronómicas X ray binaries Gamma rays Microquásars Cygnus X-1 (microcuásar) |
title_short |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
title_full |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
title_fullStr |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
title_full_unstemmed |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
title_sort |
On the nature of the episodic gamma-ray flare observed in Cygnus X-1 |
dc.creator.none.fl_str_mv |
Valle, María Victoria del Romero, Gustavo Esteban Orellana, Mariana Dominga |
author |
Valle, María Victoria del |
author_facet |
Valle, María Victoria del Romero, Gustavo Esteban Orellana, Mariana Dominga |
author_role |
author |
author2 |
Romero, Gustavo Esteban Orellana, Mariana Dominga |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Física Ciencias Astronómicas X ray binaries Gamma rays Microquásars Cygnus X-1 (microcuásar) |
topic |
Física Ciencias Astronómicas X ray binaries Gamma rays Microquásars Cygnus X-1 (microcuásar) |
dc.description.none.fl_txt_mv |
The high-mass microquasar Cygnus X-1, the best established candidate for a stellar-mass black hole, has been detected in a flaring state at very high energies, E > 200 GeV (Albert et al. 2007). The observation was per- formed by the Atmospheric Cherenkov Telescope MAGIC. It is the first experimental evidence of very high energy emission produced by a galactic stellar-mass black hole. The observed high energy excess occurred in coin- cidence with an X-ray flare. The flare took place at orbital phase = 0.91, being = 1 the moment when the black hole is behind the companion star. In this configuration the absorption of gamma-ray photons produced by photon-photon annihilation with the stellar field is expected to be the highest. We present detailed calculations of the gamma-ray opacity due to pair creation along the whole orbit, and for different locations of the emitter (height above the compact object). We discuss the location of the gamma- ray producing region in Cygnus X-1 and the energetics required to produce the flare. Facultad de Ciencias Astronómicas y Geofísicas |
description |
The high-mass microquasar Cygnus X-1, the best established candidate for a stellar-mass black hole, has been detected in a flaring state at very high energies, E > 200 GeV (Albert et al. 2007). The observation was per- formed by the Atmospheric Cherenkov Telescope MAGIC. It is the first experimental evidence of very high energy emission produced by a galactic stellar-mass black hole. The observed high energy excess occurred in coin- cidence with an X-ray flare. The flare took place at orbital phase = 0.91, being = 1 the moment when the black hole is behind the companion star. In this configuration the absorption of gamma-ray photons produced by photon-photon annihilation with the stellar field is expected to be the highest. We present detailed calculations of the gamma-ray opacity due to pair creation along the whole orbit, and for different locations of the emitter (height above the compact object). We discuss the location of the gamma- ray producing region in Cygnus X-1 and the energetics required to produce the flare. |
publishDate |
2009 |
dc.date.none.fl_str_mv |
2009-09 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/99098 |
url |
http://sedici.unlp.edu.ar/handle/10915/99098 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/23361 info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2009BAAA...52..259D info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/b52/2009BAAA...52..259D.pdf info:eu-repo/semantics/altIdentifier/issn/1669-9521 info:eu-repo/semantics/altIdentifier/hdl/11336/23361 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 259-262 |
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