CWNU 2645

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C3
N_50
r_50
AB 17 8.2
Summary

CWNU 2645 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 300.732 24.017 0.502 -2.286 -4.898 -1.66
Hunt & Reffert (2023) 300.729 23.941 0.491 -2.284 -4.88 17.37
Cavallo et al. (2024) 300.662 24.061 0.493
Hunt & Reffert (2024) 300.729 23.941 0.491 -2.284 -4.88 17.37
           
UCC 300.724 23.998 0.49 -2.296 -4.889 -0.904
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=11.3, logAge=7.75
Hunt & Reffert (2023) AV50=2.651, diffAV50=1.92, MOD50=11.367, logAge50=7.89
Cavallo et al. (2024) AV50=2.86, dMod50=11.44, logAge50=7.63, [Fe/H]50=0.28
Hunt & Reffert (2024) MassJ=189.278, MassTot=465.581

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2005 4.0 301.12 23.69 0.53 -2.26 -4.96 45.76 0.1