CWNU 1241

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.2 0.75 0.0 0.8
C3
N_50
r_50
AB 24 44.1
Summary

CWNU 1241 is a sparse, very loose object of high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 337.543 70.196 2.608 5.74 0.329 –
           
UCC 336.855 70.095 2.634 5.896 0.322 -16.13
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1241 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=1.1, logAge=7.85

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 37 20.0 333.42 70.14 2.68 5.18 0.92 -32.92 0.0
VDB 152 20.0 333.42 70.14 2.67 5.18 0.9 -32.92 0.64