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dc.contributor.author
Guarcello, Mario Giuseppe  
dc.contributor.author
Flaccomio, Ettore  
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Albacete Colombo, Juan Facundo  
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Almendros Abad, Víctor  
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Anastasopoulou, Konstantina  
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Andersen, M.  
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Argiroffi, C.  
dc.contributor.author
Bayo, Amelia  
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Bartlett, E.S.  
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Bastian, N.  
dc.contributor.author
De Becker, Michaël  
dc.contributor.author
Best, William M. J.  
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Bonito, R.  
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Borghese, Alice  
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Calzetti, D.  
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Castellanos, R.  
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Cecchi Pestellini, C.  
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Clark, J. S.  
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Clarke, C. J.  
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Zelati, Francesco Coti  
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Damiani, Jeremy  
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Drake, J.J.  
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Gennaro, Mario  
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Mapelli, M.  
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Martinez Galarza, J. R.  
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Micela, G.  
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Miceli, M.  
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Moraux, E.  
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Winter, A.  
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Wright, N. J.  
dc.contributor.author
Zeidler, Peter  
dc.date.available
2024-07-23T15:09:21Z  
dc.date.issued
2024-02  
dc.identifier.citation
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  
dc.identifier.issn
0004-6361  
dc.identifier.uri
http://hdl.handle.net/11336/240691  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
EDP Sciences  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: WESTERLUND 1  
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STARS: FORMATION  
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STARS: LOW-MASS  
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STARS: MASSIVE  
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STARS: WOLF-RAYET  
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X-RAYS: STARS  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
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info:eu-repo/semantics/publishedVersion  
dc.date.updated
2024-03-19T14:29:05Z  
dc.journal.volume
682  
dc.journal.number
A49  
dc.journal.pagination
1-22  
dc.journal.pais
Francia  
dc.description.fil
Fil: Guarcello, Mario Giuseppe. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Flaccomio, Ettore. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Albacete Colombo, Juan Facundo. Universidad Nacional de Río Negro; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina  
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Fil: Almendros Abad, Víctor. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Anastasopoulou, Konstantina. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Andersen, M.. European Southern Observatory; Alemania  
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Fil: Argiroffi, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia  
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Fil: Bayo, Amelia. European Southern Observatory; Alemania  
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Fil: Bartlett, E.S.. European Southern Observatory; Alemania  
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Fil: Bastian, N.. Donostia International Physics Center; España. Basque Foundation For Science; España. Liverpool John Moores University; Reino Unido  
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Fil: De Becker, Michaël. Université de Liège; Bélgica  
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Fil: Best, William M. J.. University of Texas at Austin; Estados Unidos  
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Fil: Bonito, R.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Borghese, Alice. Instituto de Astrofísica de Canarias; España. Universidad de La Laguna; España  
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Fil: Calzetti, D.. University of Massachusetts; Estados Unidos  
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Fil: Castellanos, R.. Centro de Astrobiología; España. Consejo Superior de Investigaciones Científicas; España  
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Fil: Cecchi Pestellini, C.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Clark, J. S.. The Open University; Reino Unido  
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Fil: Clarke, C. J.. University of Cambridge; Estados Unidos  
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Fil: Zelati, Francesco Coti. Instituto de Estudios Espaciales de Cataluña; España. Consejo Superior de Investigaciones Científicas; España  
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Fil: Damiani, Jeremy. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Drake, J.J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos  
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Fil: Gennaro, Mario. Space Telescope Science Institute; Estados Unidos. University Johns Hopkins; Estados Unidos  
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Fil: Mapelli, M.. Università di Padova; Italia. Ruprecht Karls Universitat Heidelberg; Alemania  
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Fil: Martinez Galarza, J. R.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos  
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Fil: Micela, G.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia  
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Fil: Miceli, M.. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia. Università degli Studi di Palermo; Italia  
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Fil: Moraux, E.. Universite Grenoble Alpes; Francia  
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Fil: Winter, A.. Observatoire de la Côte D'azur; Francia. Universite Grenoble Alpes; Francia  
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Fil: Wright, N. J.. Keele University; Reino Unido  
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Fil: Zeidler, Peter. European Southern Observatory; Alemania. Space Telescope Science Institute; Estados Unidos  
dc.journal.title
Astronomy and Astrophysics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/202347778  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2024/02/aa47778-23/aa47778-23.html