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Figure 1: Distribution of the COCD clusters over magnitude of the brightest star among the most probable cluster members a), over number of most probable members in a cluster b), over angular radius of a cluster c). The hatched histograms in b) and c) are for core radii, whereas the filled histograms are related to corona radii. For convenience, long tails in the distributions in b) and c) are truncated. |
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Figure 2:
Example of the spatial, kinematical and evolutionary parameters of
the new open cluster ASCC 13. Left upper panel is a sky map of the cluster
neighbourhood. The small circles are stars, their size indicates
stellar magnitude (only in this panel).
In all other diagrams stars are shown as grey dots.
The error bars indicate the rms-errors in the corresponding data for
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Figure 3:
Open clusters identified with ASCC-2.5 data: the comparison of
previously known (COCD) and newly discovered
(COCD Extension) clusters. Panel a) shows the distribution of clusters over
the sky. The crosses indicate known clusters, the circles are for newly
discovered ones. Histograms b)- f) are normalised to the number of known
clusters (
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