HSC 1866

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0.20 UTI
0.0
CN
0.52
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.52 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1866 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 114.802 -18.942 0.268 -1.734 2.31 67.756
Hunt & Reffert 2024 114.797 -18.945 0.252 -1.714 2.302 –
Cavallo et al. 2024 114.803 -19.001 0.254 – – –
Hunt & Reffert 2023 114.797 -18.945 0.252 -1.714 2.302 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 255* – –
Cavallo et al. 2024 3.12 1.13 – 257 -0.030 – – –
Hunt & Reffert 2023 3.40 1.44 0.87 96 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3760 72.0 114.8 -18.94 0.26 -1.76 2.33 67.76 0.16

💡 Note: The % column shows the percentage of members that HSC 1866 shares with each listed object.

Visualization

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