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The Young Star Clusters in S106
1994Near-infrared imaging of a 10 × 10 arcmin region of the S106 molecular cloud reveals two embedded clusters coinciding with peaks in the CO emission. By counting foreground stars seen towards the molecular cloud, the distance to S106 is found to be 1.2±0.2 kpc. Assuming a theoretical mass-luminosity relationship for pre-main sequence stars, we find that
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Search for B[e] Stars in Young Open Clusters
1998The properties and the stellar content of five young open clusters have been investigated to identify new B[e] stars. After a detailed analysis we conclude that none of the ~ 260 relatively young early type stars can be identified as such. We propose that either the B[e] characteristic is not present in young stars or that due to the close proximity of
de Winter, D. +2 more
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Model based clustering for young star clusters
2018Model based clustering is a method of fitting finite mixtures models to data in order to identify clusters. It is widely used in many fields and has a variety of applications,one of those is the identification of young star clusters. We will examine four different models multivariate Gaussian, t, Skew Normal and Skew t mixtures and a method that ...
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Intermediate mass black hole formation in compact young massive star clusters
Monthly Notices of the Royal Astronomical Society, 2021Thorsten Naab +2 more
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Young, Massive Star Clusters in the Antennae
2008While massive star clusters have been detected in almost every galaxy with appreciable star formation, they are most prevalent in interacting and merging galaxies. As many as 95% of these clusters will ultimately be disrupted, often in the first 10 Myr, but those clusters that do survive may be the progenitors of globular clusters.
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Binary black holes in young star clusters: the impact of metallicity
Monthly Notices of the Royal Astronomical Society, 2020Ugo N Di Carlo +2 more
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The spatial relation between young star clusters and molecular clouds in M51 with LEGUS
Monthly Notices of the Royal Astronomical Society, 2019Kathryn Grasha +2 more
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