EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey

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Título: EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey
Autor/es: Guarcello, Mario Giuseppe | Flaccomio, E. | Albacete-Colombo, J. F. | Almendros-Abad, Víctor | Anastasopoulou, Konstantina | Andersen, M. | Argiroffi, C. | Bayo, A. | Bartlett, Elizabeth S. | Bastian, N. | De Becker, Michaël | Best, William | Bonito, R. | Borghese, Alice | Calzetti, D. | Castellanos, Raul | Cecchi-Pestellini, C. | Clark, J. Simon | Clarke, C.J. | Coti Zelati, Francesco | Damiani, F. | Drake, J.J. | Gennaro, Mario | Ginsburg, A. | Grebel, E.K. | Hora, Joseph L. | Israel, Gian Luca | Lawrence, Grace | Locci, D. | Mapelli, M. | Martinez-Galarza, J.R. | Micela, G. | Miceli, M. | Moraux, E. | Muzic, K. | Najarro de la Parra, Francisco | Negueruela, Ignacio | Nota, A. | Pallanca, C. | Prisinzano, L. | Ritchie, Benedict | Robberto, M. | Rom, Tamara | Sabbi, Elena | Scholz, A. | Sciortino, Salvatore | Trigilio, Corrado | Umana, G. | Winter, A. | Wright, N.J. | Zeidler, Peter
Grupo/s de investigación o GITE: Astrofísica Estelar (AE)
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física Aplicada
Palabras clave: Stars: formation | Stars: low-mass | Stars: massive | Stars: Wolf-Rayet | X-rays: stars | Open clusters and associations: individual: Westerlund 1
Fecha de publicación: 2-feb-2024
Editor: EDP Sciences
Cita bibliográfica: Astronomy & Astrophysics. 2024, 682: A49. https://doi.org/10.1051/0004-6361/202347778
Resumen: 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.
Patrocinador/es: M.G.G., C.A., R.B., E.F., G.L.I., L.P., and S.S. acknowledge the INAF grant 1.05.12.05.03. K.M. acknowledges support from the Fundação para a Ciência e a Tecnologia (FCT) through the CEEC-individual contract 2022.03809.CEECIND and research grants UIDB/04434/2020 and UIDP/04434/2020. Support for this work was also provided by the National Aeronautics and Space Administration through Chandra Proposal 21200267 issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060. I.N. is partially supported by the Spanish Government Ministerio de Ciencia e Innovación (MCIN) and Agencia Estatal de Investigación (MCIN/AEI/10.130 39/501 100 011 033/FEDER, UE) under grant PID2021-122397NB-C22, and also by MCIN with funding from the European Union NextGenerationEU and Generalitat Valenciana in the call Programa de Planes Complementarios de I+D+i (PRTR 2022), project HIAMAS, reference ASFAE/2022/017. M. G. G. and R. B. acknowledge partial support from the Grant INAF 2022 YODA; R. B. also acknowledges partial support from the project PRIN-INAF 2019 “Spectroscopically Tracing the Disk Dispersal Evolution”. The scientific results reported in this article are based on observations made by the Chandra X-ray Observatory. M.M. acknowledges financial support from the European Research Council for the ERC Consolidator grant DEMOBLACK, under contract no. 770017, and from the German Excellence Strategy via the Heidelberg Cluster of Excellence (EXC 2181 – 390900948) STRUCTURES.
URI: http://hdl.handle.net/10045/140758
ISSN: 0004-6361 (Print) | 1432-0746 (Online)
DOI: 10.1051/0004-6361/202347778
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: © The Authors 2024. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Revisión científica: si
Versión del editor: https://doi.org/10.1051/0004-6361/202347778
Aparece en las colecciones:INV - Astrofísica Estelar - Artículos de Revistas
Investigaciones financiadas por la UE

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