CWNU 1749

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C3
N_50
r_50
CB 29 5.4
Summary

CWNU 1749 is a poorly populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 2.482 60.382 0.438 -2.164 -1.377
Hunt & Reffert (2023) 2.489 60.414 0.437 -2.146 -1.4 -41.292
Cavallo et al. (2024) 2.448 60.403 0.439
Hunt & Reffert (2024) 2.489 60.414 0.437 -2.146 -1.4 -41.292
           
UCC 2.491 60.387 0.438 -2.163 -1.391 -42.123
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=1.6, m-M=11.65, logAge=7.7
Hunt & Reffert (2023) AV50=1.123, diffAV50=0.694, MOD50=11.687, logAge50=8.224
Cavallo et al. (2024) AV50=1.03, dMod50=11.43, logAge50=8.39, [Fe/H]50=0.17
Hunt & Reffert (2024) MassJ=143.281, MassTot=147.116

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Cluster region map