HSC 2278

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C3
N_50
r_50
DB 26 195.6
Summary

HSC 2278 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

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) 172.153 -24.589 7.976 -9.356 0.728 1.308
Cavallo et al. (2024) 169.663 -23.463 7.944
Hu & Soubiran (2025) 169.663 -23.463
           
UCC 169.079 -25.051 7.861 -9.271 0.677 2.209
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=0.092, diffAV50=0.288, MOD50=5.389, logAge50=8.756
Cavallo et al. (2024) AV50=0.44, dMod50=5.55, logAge50=9.18, [Fe/H]50=0.08
Hu & Soubiran (2025) MA22=-0.26, MA23f=-0.33, MZ23=-0.07, MK24=-0.09, MF24=-0.5

Search coordinates in Bayestar19

Cluster region map