On the existence of young embedded clusters at high Galactic latitude

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dc.contributor.authorTurner, D. G.
dc.contributor.authorCarraro, G.
dc.contributor.authorPanko, Olena O.
dc.contributor.authorПанько, Олена Олексіївна
dc.contributor.authorПанько, Елена Алексеевна
dc.date.accessioned2019-05-16T07:36:46Z
dc.date.available2019-05-16T07:36:46Z
dc.date.issued2017
dc.description.abstractCareful analyses of photometric and star count data available for the nine putative young clusters identified by Camargo et al. (2015, 2016) at high Galactic latitudes reveal that none of the groups contain early-type stars, and most are not significant density enhancements above field level. 2MASS colours for stars in the groups match those of unreddened late-type dwarfs and giants, as expected for contamination by (mostly) thin disk objects. A simulation of one such field using only typical high latitude foreground stars yields a colour-magnitude diagram that is very similar to those constructed by Camargo et al. (2015, 2016) as evidence for their young groups as well as the means of deriving their reddenings and distances. Although some of the fields are coincident with clusters of galaxies, one must conclude that there is no evidence that the putative clusters are extremely young stellar groups.uk_UA
dc.identifier.citationMonthly Notices of the Royal Astronomical Societyuk_UA
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/24038
dc.language.isoenuk_UA
dc.relation.ispartofseries;Vol. 470, іssue 1.
dc.subjectAstronomical techniquesuk_UA
dc.subjectphotometric — Galaxyuk_UA
dc.subjectopen clusters and associationsuk_UA
dc.subjectgeneral — infrared: generaluk_UA
dc.titleOn the existence of young embedded clusters at high Galactic latitudeuk_UA
dc.typeArticleuk_UA
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