CWNU 1780

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C3
N_50
r_50
BB 24 3.0
Summary

CWNU 1780 is a sparse, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

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) 5.722 62.239 0.466 -2.847 -1.629
Hunt & Reffert (2023) 5.726 62.239 0.467 -2.856 -1.63
Cavallo et al. (2024) 5.756 62.243 0.467
Hunt & Reffert (2024) 5.726 62.239 0.467 -2.856 -1.63
           
UCC 5.709 62.238 0.467 -2.85 -1.628
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=11.6, logAge=6.9
Hunt & Reffert (2023) AV50=1.028, diffAV50=0.767, MOD50=11.498, logAge50=6.899
Cavallo et al. (2024) AV50=1.21, dMod50=11.55, logAge50=6.65, [Fe/H]50=0.02
Hunt & Reffert (2024) MassJ=236.549, MassTot=243.511

Search coordinates in Bayestar19

Cluster region map