HSC 1750

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C3
N_50
r_50
BB 59 5.0
Summary

HSC 1750 is a moderately populated, moderately dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 103.487 -9.945 0.311 -0.27 -1.119 53.113
Cavallo et al. (2024) 103.467 -9.931 0.312
Hunt & Reffert (2024) 103.487 -9.945 0.311 -0.27 -1.119 53.113
Hu & Soubiran (2025) 103.467 -9.931
           
UCC 103.495 -9.939 0.307 -0.27 -1.122 53.118
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
Hunt & Reffert (2023) AV50=1.616, diffAV50=1.864, MOD50=12.2, logAge50=8.627
Cavallo et al. (2024) AV50=1.58, dMod50=11.66, logAge50=8.99, [Fe/H]50=-0.23
Hunt & Reffert (2024) MassJ=370.329, MassTot=433.184
Hu & Soubiran (2025) MA22=-0.24, MA23f=-0.35, MZ23=-0.32, MK24=-0.25, MF24=-0.34

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2982 52.5 103.49 -9.94 0.31 -0.27 -1.12 53.12 0.0