HSC 1749

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C3
N_50
r_50
CC 27 11.8
Summary

HSC 1749 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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) 105.141 -9.027 0.363 -1.883 2.23
Cavallo et al. (2024) 105.114 -8.9 0.361
           
UCC 105.135 -9.031 0.349 -1.901 2.267
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=1.206, diffAV50=1.598, MOD50=11.952, logAge50=8.027
Cavallo et al. (2024) AV50=0.74, dMod50=12.43, logAge50=8.3, [Fe/H]50=0.35

Search coordinates in Bayestar19

Cluster region map