HSC 1752

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.05 0.38 0.0 0.4
C3
N_50
r_50
BC 17 10.1
Summary

HSC 1752 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously 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=0.4) 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) 107.835 -8.409 0.349 -1.195 1.008 –
Cavallo et al. (2024) 107.829 -8.371 0.35 – – –
           
UCC 107.815 -8.394 0.371 -1.215 1.0 97.513
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

HSC 1752 UCC
HSC 1752 HUNT23

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Fundamental parameters

Reference Values
Hunt & Reffert (2023) AV50=0.689, diffAV50=1.107, MOD50=11.988, logAge50=7.668
Cavallo et al. (2024) AV50=0.9, dMod50=11.97, logAge50=7.07, [Fe/H]50=-0.35

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 171 60.0 107.84 -8.4 0.34 -1.2 1.01 82.55 0.1