Clustered star formation toward Berkeley 87/ON2 - I. Multiwavelength census and the population overlap problem

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Título: Clustered star formation toward Berkeley 87/ON2 - I. Multiwavelength census and the population overlap problem
Autor/es: de la Fuente, Diego | Román-Zúñiga, Carlos G. | Jiménez-Bailón, Elena | Alves, João | García, Miriam | Venus, Sean
Grupo/s de investigación o GITE: Astrofísica Estelar (AE)
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal
Palabras clave: Methods: observational | Techniques: photometric | Catalogs | Open clusters and associations: individual: Berkeley 87 | ISM: individual objects: ON2 | Stars: formation
Área/s de conocimiento: Física Aplicada
Fecha de publicación: 24-jun-2021
Editor: EDP Sciences
Cita bibliográfica: Astronomy & Astrophysics. 2021, 650: A156. https://doi.org/10.1051/0004-6361/202040065
Resumen: Context. Disentangling line-of-sight alignments of young stellar populations is crucial for observational studies of star-forming complexes. This task is particularly problematic in a Cygnus-X subregion where several components, located at different distances, overlap: the Berkeley 87 young massive cluster, the poorly known [DB2001] Cl05 embedded cluster, and the ON2 star-forming complex, which in turn is composed of several H II regions. Aims. We provide a methodology for building an exhaustive census of young objects that can consistently treat large differences in extinction and distance. Methods. OMEGA2000 near-infrared observations of the Berkeley 87/ON2 field were merged with archival data from Gaia, Chandra, Spitzer, and Herschel and with cross-identifications from the literature. To address the incompleteness effects and selection biases that arise from the line-of-sight overlap, we adapted existing methods for extinction estimation and young object classification. We also defined the intrinsic reddening index, Rint, a new tool for separating intrinsically red sources from those whose infrared color excess is caused by extinction. Finally, we introduce a new method for finding young stellar objects based on Rint. Results. We find 571 objects whose classification is related to recent or ongoing star formation. Together with other point sources with individual estimates of distance or extinction, we compile a catalog of 3005 objects to be used for further membership work. A new distance for Berkeley 87, (1673 ± 17) pc, is estimated as a median of 13 spectroscopic members with accurate Gaia EDR3 parallaxes. Conclusions. The flexibility of our approach, especially regarding the Rint definition, allows overcoming photometric biases caused by large variations in extinction and distance in order to obtain homogeneous catalogs of young sources. The multiwavelength census that results from applying our methods to the Berkeley 87/ON2 field will serve as a basis for disentangling the overlapped populations.
Patrocinador/es: D.dF. acknowledges the UNAM-DGAPA postdoctoral grant, the Generalitat Valenciana APOSTD/220/228 fellowship, and the Spanish Government AYA2015-68012-C2-2-P project. D.dF. and M.G. have received financial support from Spanish Government project ESP2017-86582-C4-1-R. C.R.-Z. acknowledges support from CONACYT project CB2017-2018 A1-S-9754. C.R.-Z. and E.J.B. acknowledge support from Programa de Apoyo a Proyectos de Investigación e Innovación Tecnológica, UNAM-DGAPA, grants IN108117 and IN109217, respectively.
URI: http://hdl.handle.net/10045/116355
ISSN: 0004-6361 (Print) | 1432-0746 (Online)
DOI: 10.1051/0004-6361/202040065
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: © ESO 2021
Revisión científica: si
Versión del editor: https://doi.org/10.1051/0004-6361/202040065
Aparece en las colecciones:INV - Astrofísica Estelar - Artículos de Revistas

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