EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey
- Autores
- Guarcello, Mario Giuseppe; Flaccomio, Ettore; Albacete Colombo, Juan Facundo; Almendros Abad, Víctor; Anastasopoulou, Konstantina; Andersen, M.; Argiroffi, C.; Bayo, Amelia; Bartlett, E.S.; Bastian, N.; De Becker, Michaël; Best, William M. J.; Bonito, R.; Borghese, Alice; Calzetti, D.; Castellanos, R.; Cecchi Pestellini, C.; Clark, J. S.; Clarke, C. J.; Zelati, Francesco Coti; Damiani, Jeremy; Drake, J.J.; Gennaro, Mario; Mapelli, M.; Martinez Galarza, J. R.; Micela, G.; Miceli, M.; Moraux, E.; Winter, A.; Wright, N. J.; Zeidler, Peter
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s −1 . The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
Fil: Guarcello, Mario Giuseppe. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Flaccomio, Ettore. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Albacete Colombo, Juan Facundo. Universidad Nacional de Río Negro; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Almendros Abad, Víctor. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Anastasopoulou, Konstantina. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Andersen, M.. European Southern Observatory; Alemania
Fil: Argiroffi, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia
Fil: Bayo, Amelia. European Southern Observatory; Alemania
Fil: Bartlett, E.S.. European Southern Observatory; Alemania
Fil: Bastian, N.. Donostia International Physics Center; España. Basque Foundation For Science; España. Liverpool John Moores University; Reino Unido
Fil: De Becker, Michaël. Université de Liège; Bélgica
Fil: Best, William M. J.. University of Texas at Austin; Estados Unidos
Fil: Bonito, R.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Borghese, Alice. Instituto de Astrofísica de Canarias; España. Universidad de La Laguna; España
Fil: Calzetti, D.. University of Massachusetts; Estados Unidos
Fil: Castellanos, R.. Centro de Astrobiología; España. Consejo Superior de Investigaciones Científicas; España
Fil: Cecchi Pestellini, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Clark, J. S.. The Open University; Reino Unido
Fil: Clarke, C. J.. University of Cambridge; Estados Unidos
Fil: Zelati, Francesco Coti. Instituto de Estudios Espaciales de Cataluña; España. Consejo Superior de Investigaciones Científicas; España
Fil: Damiani, Jeremy. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Drake, J.J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Gennaro, Mario. Space Telescope Science Institute; Estados Unidos. University Johns Hopkins; Estados Unidos
Fil: Mapelli, M.. Università di Padova; Italia. Ruprecht Karls Universitat Heidelberg; Alemania
Fil: Martinez Galarza, J. R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Micela, G.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Miceli, M.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia
Fil: Moraux, E.. Universite Grenoble Alpes; Francia
Fil: Winter, A.. Observatoire de la Côte D'azur; Francia. Universite Grenoble Alpes; Francia
Fil: Wright, N. J.. Keele University; Reino Unido
Fil: Zeidler, Peter. European Southern Observatory; Alemania. Space Telescope Science Institute; Estados Unidos - Materia
-
OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1
STARS: FORMATION
STARS: LOW-MASS
STARS: MASSIVE
STARS: WOLF-RAYET
X-RAYS: STARS - 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:11336/240691
Ver los metadatos del registro completo
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EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters SurveyGuarcello, Mario GiuseppeFlaccomio, EttoreAlbacete Colombo, Juan FacundoAlmendros Abad, VíctorAnastasopoulou, KonstantinaAndersen, M.Argiroffi, C.Bayo, AmeliaBartlett, E.S.Bastian, N.De Becker, MichaëlBest, William M. J.Bonito, R.Borghese, AliceCalzetti, D.Castellanos, R.Cecchi Pestellini, C.Clark, J. S.Clarke, C. J.Zelati, Francesco CotiDamiani, JeremyDrake, J.J.Gennaro, MarioMapelli, M.Martinez Galarza, J. R.Micela, G.Miceli, M.Moraux, E.Winter, A.Wright, N. J.Zeidler, PeterOPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1STARS: FORMATIONSTARS: LOW-MASSSTARS: MASSIVESTARS: WOLF-RAYETX-RAYS: STARShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s −1 . The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.Fil: Guarcello, Mario Giuseppe. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Flaccomio, Ettore. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Albacete Colombo, Juan Facundo. Universidad Nacional de Río Negro; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Almendros Abad, Víctor. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Anastasopoulou, Konstantina. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Andersen, M.. European Southern Observatory; AlemaniaFil: Argiroffi, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; ItaliaFil: Bayo, Amelia. European Southern Observatory; AlemaniaFil: Bartlett, E.S.. European Southern Observatory; AlemaniaFil: Bastian, N.. Donostia International Physics Center; España. Basque Foundation For Science; España. Liverpool John Moores University; Reino UnidoFil: De Becker, Michaël. Université de Liège; BélgicaFil: Best, William M. J.. University of Texas at Austin; Estados UnidosFil: Bonito, R.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Borghese, Alice. Instituto de Astrofísica de Canarias; España. Universidad de La Laguna; EspañaFil: Calzetti, D.. University of Massachusetts; Estados UnidosFil: Castellanos, R.. Centro de Astrobiología; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Cecchi Pestellini, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Clark, J. S.. The Open University; Reino UnidoFil: Clarke, C. J.. University of Cambridge; Estados UnidosFil: Zelati, Francesco Coti. Instituto de Estudios Espaciales de Cataluña; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Damiani, Jeremy. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Drake, J.J.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Gennaro, Mario. Space Telescope Science Institute; Estados Unidos. University Johns Hopkins; Estados UnidosFil: Mapelli, M.. Università di Padova; Italia. Ruprecht Karls Universitat Heidelberg; AlemaniaFil: Martinez Galarza, J. R.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Micela, G.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Miceli, M.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; ItaliaFil: Moraux, E.. Universite Grenoble Alpes; FranciaFil: Winter, A.. Observatoire de la Côte D'azur; Francia. Universite Grenoble Alpes; FranciaFil: Wright, N. J.. Keele University; Reino UnidoFil: Zeidler, Peter. European Southern Observatory; Alemania. Space Telescope Science Institute; Estados UnidosEDP Sciences2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/240691Guarcello, Mario Giuseppe; Flaccomio, Ettore; Albacete Colombo, Juan Facundo; Almendros Abad, Víctor; Anastasopoulou, Konstantina; et al.; EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey; EDP Sciences; Astronomy and Astrophysics; 682; A49; 2-2024; 1-220004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202347778info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2024/02/aa47778-23/aa47778-23.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:00:50Zoai:ri.conicet.gov.ar:11336/240691instacron: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:34982025-09-10 13:00:51.185CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| title |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| spellingShingle |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey Guarcello, Mario Giuseppe OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1 STARS: FORMATION STARS: LOW-MASS STARS: MASSIVE STARS: WOLF-RAYET X-RAYS: STARS |
| title_short |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| title_full |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| title_fullStr |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| title_full_unstemmed |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| title_sort |
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey |
| dc.creator.none.fl_str_mv |
Guarcello, Mario Giuseppe Flaccomio, Ettore Albacete Colombo, Juan Facundo Almendros Abad, Víctor Anastasopoulou, Konstantina Andersen, M. Argiroffi, C. Bayo, Amelia Bartlett, E.S. Bastian, N. De Becker, Michaël Best, William M. J. Bonito, R. Borghese, Alice Calzetti, D. Castellanos, R. Cecchi Pestellini, C. Clark, J. S. Clarke, C. J. Zelati, Francesco Coti Damiani, Jeremy Drake, J.J. Gennaro, Mario Mapelli, M. Martinez Galarza, J. R. Micela, G. Miceli, M. Moraux, E. Winter, A. Wright, N. J. Zeidler, Peter |
| author |
Guarcello, Mario Giuseppe |
| author_facet |
Guarcello, Mario Giuseppe Flaccomio, Ettore Albacete Colombo, Juan Facundo Almendros Abad, Víctor Anastasopoulou, Konstantina Andersen, M. Argiroffi, C. Bayo, Amelia Bartlett, E.S. Bastian, N. De Becker, Michaël Best, William M. J. Bonito, R. Borghese, Alice Calzetti, D. Castellanos, R. Cecchi Pestellini, C. Clark, J. S. Clarke, C. J. Zelati, Francesco Coti Damiani, Jeremy Drake, J.J. Gennaro, Mario Mapelli, M. Martinez Galarza, J. R. Micela, G. Miceli, M. Moraux, E. Winter, A. Wright, N. J. Zeidler, Peter |
| author_role |
author |
| author2 |
Flaccomio, Ettore Albacete Colombo, Juan Facundo Almendros Abad, Víctor Anastasopoulou, Konstantina Andersen, M. Argiroffi, C. Bayo, Amelia Bartlett, E.S. Bastian, N. De Becker, Michaël Best, William M. J. Bonito, R. Borghese, Alice Calzetti, D. Castellanos, R. Cecchi Pestellini, C. Clark, J. S. Clarke, C. J. Zelati, Francesco Coti Damiani, Jeremy Drake, J.J. Gennaro, Mario Mapelli, M. Martinez Galarza, J. R. Micela, G. Miceli, M. Moraux, E. Winter, A. Wright, N. J. Zeidler, Peter |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1 STARS: FORMATION STARS: LOW-MASS STARS: MASSIVE STARS: WOLF-RAYET X-RAYS: STARS |
| topic |
OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1 STARS: FORMATION STARS: LOW-MASS STARS: MASSIVE STARS: WOLF-RAYET X-RAYS: STARS |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s −1 . The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217. Fil: Guarcello, Mario Giuseppe. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Flaccomio, Ettore. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Albacete Colombo, Juan Facundo. Universidad Nacional de Río Negro; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Almendros Abad, Víctor. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Anastasopoulou, Konstantina. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Andersen, M.. European Southern Observatory; Alemania Fil: Argiroffi, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia Fil: Bayo, Amelia. European Southern Observatory; Alemania Fil: Bartlett, E.S.. European Southern Observatory; Alemania Fil: Bastian, N.. Donostia International Physics Center; España. Basque Foundation For Science; España. Liverpool John Moores University; Reino Unido Fil: De Becker, Michaël. Université de Liège; Bélgica Fil: Best, William M. J.. University of Texas at Austin; Estados Unidos Fil: Bonito, R.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Borghese, Alice. Instituto de Astrofísica de Canarias; España. Universidad de La Laguna; España Fil: Calzetti, D.. University of Massachusetts; Estados Unidos Fil: Castellanos, R.. Centro de Astrobiología; España. Consejo Superior de Investigaciones Científicas; España Fil: Cecchi Pestellini, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Clark, J. S.. The Open University; Reino Unido Fil: Clarke, C. J.. University of Cambridge; Estados Unidos Fil: Zelati, Francesco Coti. Instituto de Estudios Espaciales de Cataluña; España. Consejo Superior de Investigaciones Científicas; España Fil: Damiani, Jeremy. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Drake, J.J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Gennaro, Mario. Space Telescope Science Institute; Estados Unidos. University Johns Hopkins; Estados Unidos Fil: Mapelli, M.. Università di Padova; Italia. Ruprecht Karls Universitat Heidelberg; Alemania Fil: Martinez Galarza, J. R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Micela, G.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Miceli, M.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia Fil: Moraux, E.. Universite Grenoble Alpes; Francia Fil: Winter, A.. Observatoire de la Côte D'azur; Francia. Universite Grenoble Alpes; Francia Fil: Wright, N. J.. Keele University; Reino Unido Fil: Zeidler, Peter. European Southern Observatory; Alemania. Space Telescope Science Institute; Estados Unidos |
| description |
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s −1 . The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217. |
| publishDate |
2024 |
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2024-02 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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http://hdl.handle.net/11336/240691 Guarcello, Mario Giuseppe; Flaccomio, Ettore; Albacete Colombo, Juan Facundo; Almendros Abad, Víctor; Anastasopoulou, Konstantina; et al.; EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey; EDP Sciences; Astronomy and Astrophysics; 682; A49; 2-2024; 1-22 0004-6361 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/240691 |
| identifier_str_mv |
Guarcello, Mario Giuseppe; Flaccomio, Ettore; Albacete Colombo, Juan Facundo; Almendros Abad, Víctor; Anastasopoulou, Konstantina; et al.; EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey; EDP Sciences; Astronomy and Astrophysics; 682; A49; 2-2024; 1-22 0004-6361 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202347778 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2024/02/aa47778-23/aa47778-23.html |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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