CWNU 311

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C3
N_50
r_50
CA 22 30.4
Summary

CWNU 311 is a sparse, very loose object of intermediate C3 quality. It is located at a close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a moderate 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. (2022) 332.775 42.341 1.56 -1.11 -4.52 -0.6
Hunt & Reffert (2023) 333.434 42.479 1.553 -1.133 -4.475 -6.716
Cavallo et al. (2024) 332.749 42.552 1.548
           
UCC 332.91 42.375 1.557 -1.139 -4.523 -10.475
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.35, m-M=9.0, logAge=7.5, Z=0.022
Hunt & Reffert (2023) AV50=0.623, diffAV50=1.12, MOD50=8.999, logAge50=7.691
Cavallo et al. (2024) AV50=0.84, dMod50=9.16, logAge50=7.06, [Fe/H]50=-0.06

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 294 32.0 334.61 42.99 1.59 -0.98 -4.38 -8.62 0.25