The young open clusters King 12, NGC 7788, and NGC 7790: pre-main-sequence stars and extended stellar halos

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DOITrouver le DOI : http://doi.org/10.1088/0004-637X/761/2/155
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TypeArticle
Titre de la revueThe Astrophysical Journal
ISSN0004-637X
Volume761
Numéro2
Numéro d'article155
RésuméThe stellar contents of the open clusters King 12, NGC 7788, and NGC 7790 are investigated using MegaCam images. Comparisons with isochrones yield an age <20 Myr for King 12, 20-40 Myr for NGC 7788, and 60-80 Myr for NGC 7790 based on the properties of stars near the main-sequence turnoff (MSTO) in each cluster. The reddening of NGC 7788 is much larger than previously estimated. The luminosity functions (LFs) of King 12 and NGC 7788 show breaks that are attributed to the onset of pre-main-sequence (PMS) objects, and comparisons with models of PMS evolution yield ages that are consistent with those measured from stars near the MSTO. In contrast, the r′ LF of main-sequence stars in NGC 7790 is matched to r′ = 20 by a model that is based on the solar neighborhood mass function. The structural properties of all three clusters are investigated by examining the two-point angular correlation function of blue main-sequence stars. King 12 and NGC 7788 are each surrounded by a stellar halo that extends out to a radius of 5 arcmin (∼3.4 pc). It is suggested that these halos form in response to large-scale mass ejection early in the evolution of the clusters, as predicted by models. In contrast, blue main-sequence stars in NGC 7790 are traced out to a radius of ∼7.5 arcmin (∼5.5 pc), with no evidence of a halo. It is suggested that all three clusters may have originated in the same star-forming complex, but not in the same giant molecular cloud. © 2012. The American Astronomical Society. All rights reserved..
Date de publication
Langueanglais
AffiliationInfrastructure scientifique nationale; Conseil national de recherches Canada
Publications évaluées par des pairsOui
Numéro NPARC21270048
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Identificateur de l’enregistrementade51a7f-39d1-4d08-8754-75e704e837e8
Enregistrement créé2013-12-16
Enregistrement modifié2016-05-09
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