CWNU 1770

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.29 1.0 1.0 0.0 0.24
C3
N_50
r_50
AA 29 2.9
Summary

CWNU 1770 is a poorly populated, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 273.174 -24.363 0.739 1.612 -1.402 –
           
UCC 273.195 -24.374 0.729 1.601 -1.407 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1770 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.2, m-M=10.75, logAge=6.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
ESO 522 05 75.9 273.19 -24.35 0.73 1.61 -1.43 -36.25 0.62