CWNU 2750

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C3
N_50
r_50
AB 45 7.3
Summary

CWNU 2750 is a poorly populated, loose object of high C3 quality. It is located at a moderate distance from the Sun, near 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 186.973 -61.979 0.457 -5.199 -0.206
Hunt & Reffert (2023) 186.971 -61.986 0.451 -5.227 -0.209 -54.748
Cavallo et al. (2024) 187.082 -61.969 0.449
Hunt & Reffert (2024) 186.971 -61.986 0.451 -5.227 -0.209 -54.748
           
UCC 186.963 -61.978 0.462 -5.195 -0.202
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=11.55, logAge=7.35
Hunt & Reffert (2023) AV50=1.388, diffAV50=1.88, MOD50=11.517, logAge50=7.645
Cavallo et al. (2024) AV50=1.72, dMod50=11.57, logAge50=7.25, [Fe/H]50=-0.12
Hunt & Reffert (2024) MassJ=272.371, MassTot=347.065

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2520 2.2 186.21 -61.79 0.46 -5.3 -0.24 0.09