HSC 381

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C3
N_50
r_50
BA 27 54.1
Summary

HSC 381 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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) 271.386 17.771 3.161 -1.036 -8.11 -17.045
Cavallo et al. (2024) 270.773 19.135 3.178
           
UCC 270.961 19.467 3.227 -1.162 -8.033 -16.73
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=0.211, diffAV50=0.827, MOD50=7.464, logAge50=7.487
Cavallo et al. (2024) AV50=0.66, dMod50=7.53, logAge50=7.22, [Fe/H]50=-0.05

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 11 3.7 270.09 21.47 3.39 -1.34 -7.63 -18.06 0.19