HSC 975

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C3
N_50
r_50
BB 23 5.2
Summary

HSC 975 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 11.162 63.805 0.279 0.268 -0.612 -30.361
Cavallo et al. (2024) 11.075 63.78 0.28
Hunt & Reffert (2024) 11.162 63.805 0.279 0.268 -0.612 -30.361
           
UCC 11.166 63.781 0.269 0.283 -0.607 -29.022
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
Hunt & Reffert (2023) AV50=2.964, diffAV50=1.825, MOD50=12.567, logAge50=8.352
Cavallo et al. (2024) AV50=3.27, dMod50=12.6, logAge50=8.68, [Fe/H]50=-0.05
Hunt & Reffert (2024) MassJ=207.620, MassTot=368.083

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3435 96.0 11.13 63.78 0.27 0.29 -0.61 -29.02 0.05