HSC 2173

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0.23 UTI
0.3
CN
0.49
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.4 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2173 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large 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.

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 135.109 -47.989 0.141 -3.281 3.34 58.13
Hunt & Reffert 2024 135.109 -47.989 0.163 -3.293 3.356 57.809
Cavallo et al. 2024 135.054 -47.986 0.159 – – –
Hunt & Reffert 2023 135.109 -47.989 0.163 -3.293 3.356 57.809

💡 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] Bfrac BSS
UCC 99999– 5.71 4.33 2.75 252 -0.110 1531 – –
Hunt & Reffert 2024 – – – – – 1531(1) – –
Cavallo et al. 2024 6.73 4.01 – 282 -0.110 – – –
Hunt & Reffert 2023 4.69 4.65 2.75 221 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3215 100.0 135.11 -47.99 0.14 -3.28 3.33 58.13 0.18

💡 Note: The % column shows the percentage of members that HSC 2173 shares with each listed object.

Visualization

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