The dark side of supergiant High-Mass X-ray Binaries

Autores
Chaty, Sylvain; Fortin, Francis; García, Federico; Fogantini, Federico Adrián
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
High Mass X-ray Binaries (HMXB) have been revealed by a wealth of multi-wavelength observations, from X-ray to optical and infrared domain. After describing the 3 different kinds of HMXB, we focus on 3 HMXB hosting supergiant stars: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848, respectively called “The Good”, “The Bad” and “The Ugly”. We review in these proceedings what the observations of these sources have brought to light concerning our knowledge of HMXB, and what part still remains in the dark side. Many questions are still pending, related to accretion processes, stellar wind properties in these massive and active stars, and the overall evolution due to transfer of mass and angular momentum between the companion star and the compact object. Future observations should be able to answer these questions, which constitute the dark side of HMXB.
Instituto Argentino de Radioastronomía
Materia
Ciencias Astronómicas
(Stars:) binaries (including multiple): close
Circumstellar matter
Early-type
Emission-line
Be
Stars: neutron
Supergiants
Winds
Outflows
(ISM:) dust
Extinction
Infrared: stars
X-rays: binaries: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/126094
Acceder
id SEDICI_a00fde779d7fc92e699e160b4eb39db1
oai_identifier_str oai:sedici.unlp.edu.ar:10915/126094
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling The dark side of supergiant High-Mass X-ray BinariesChaty, SylvainFortin, FrancisGarcía, FedericoFogantini, Federico AdriánCiencias Astronómicas(Stars:) binaries (including multiple): closeCircumstellar matterEarly-typeEmission-lineBeStars: neutronSupergiantsWindsOutflows(ISM:) dustExtinctionInfrared: starsX-rays: binaries: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848High Mass X-ray Binaries (HMXB) have been revealed by a wealth of multi-wavelength observations, from X-ray to optical and infrared domain. After describing the 3 different kinds of HMXB, we focus on 3 HMXB hosting supergiant stars: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848, respectively called “The Good”, “The Bad” and “The Ugly”. We review in these proceedings what the observations of these sources have brought to light concerning our knowledge of HMXB, and what part still remains in the dark side. Many questions are still pending, related to accretion processes, stellar wind properties in these massive and active stars, and the overall evolution due to transfer of mass and angular momentum between the companion star and the compact object. Future observations should be able to answer these questions, which constitute the dark side of HMXB.Instituto Argentino de Radioastronomía2019info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf161-169http://sedici.unlp.edu.ar/handle/10915/126094enginfo:eu-repo/semantics/altIdentifier/issn/1743-9213info:eu-repo/semantics/altIdentifier/issn/1743-9221info:eu-repo/semantics/altIdentifier/doi/10.1017/s1743921319001273info: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:UNLP2025-10-15T11:22:06Zoai:sedici.unlp.edu.ar:10915/126094Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:22:06.464SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The dark side of supergiant High-Mass X-ray Binaries
title The dark side of supergiant High-Mass X-ray Binaries
spellingShingle The dark side of supergiant High-Mass X-ray Binaries
Chaty, Sylvain
Ciencias Astronómicas
(Stars:) binaries (including multiple): close
Circumstellar matter
Early-type
Emission-line
Be
Stars: neutron
Supergiants
Winds
Outflows
(ISM:) dust
Extinction
Infrared: stars
X-rays: binaries: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848
title_short The dark side of supergiant High-Mass X-ray Binaries
title_full The dark side of supergiant High-Mass X-ray Binaries
title_fullStr The dark side of supergiant High-Mass X-ray Binaries
title_full_unstemmed The dark side of supergiant High-Mass X-ray Binaries
title_sort The dark side of supergiant High-Mass X-ray Binaries
dc.creator.none.fl_str_mv Chaty, Sylvain
Fortin, Francis
García, Federico
Fogantini, Federico Adrián
author Chaty, Sylvain
author_facet Chaty, Sylvain
Fortin, Francis
García, Federico
Fogantini, Federico Adrián
author_role author
author2 Fortin, Francis
García, Federico
Fogantini, Federico Adrián
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
(Stars:) binaries (including multiple): close
Circumstellar matter
Early-type
Emission-line
Be
Stars: neutron
Supergiants
Winds
Outflows
(ISM:) dust
Extinction
Infrared: stars
X-rays: binaries: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848
topic Ciencias Astronómicas
(Stars:) binaries (including multiple): close
Circumstellar matter
Early-type
Emission-line
Be
Stars: neutron
Supergiants
Winds
Outflows
(ISM:) dust
Extinction
Infrared: stars
X-rays: binaries: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848
dc.description.none.fl_txt_mv High Mass X-ray Binaries (HMXB) have been revealed by a wealth of multi-wavelength observations, from X-ray to optical and infrared domain. After describing the 3 different kinds of HMXB, we focus on 3 HMXB hosting supergiant stars: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848, respectively called “The Good”, “The Bad” and “The Ugly”. We review in these proceedings what the observations of these sources have brought to light concerning our knowledge of HMXB, and what part still remains in the dark side. Many questions are still pending, related to accretion processes, stellar wind properties in these massive and active stars, and the overall evolution due to transfer of mass and angular momentum between the companion star and the compact object. Future observations should be able to answer these questions, which constitute the dark side of HMXB.
Instituto Argentino de Radioastronomía
description High Mass X-ray Binaries (HMXB) have been revealed by a wealth of multi-wavelength observations, from X-ray to optical and infrared domain. After describing the 3 different kinds of HMXB, we focus on 3 HMXB hosting supergiant stars: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848, respectively called “The Good”, “The Bad” and “The Ugly”. We review in these proceedings what the observations of these sources have brought to light concerning our knowledge of HMXB, and what part still remains in the dark side. Many questions are still pending, related to accretion processes, stellar wind properties in these massive and active stars, and the overall evolution due to transfer of mass and angular momentum between the companion star and the compact object. Future observations should be able to answer these questions, which constitute the dark side of HMXB.
publishDate 2019
dc.date.none.fl_str_mv 2019
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/10915/126094
url http://sedici.unlp.edu.ar/handle/10915/126094
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1743-9213
info:eu-repo/semantics/altIdentifier/issn/1743-9221
info:eu-repo/semantics/altIdentifier/doi/10.1017/s1743921319001273
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)
dc.format.none.fl_str_mv application/pdf
161-169
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.22299

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