HSC 1876

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0.10 UTI
0.25
CN
0.11
Cdens
0.75
CC3
0.03
Clit
0.44
Cdup
Core radius and density 1.7 [pc], 0.5 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.11 Very loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 0.44 Possibly duplicate

Overview

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HSC 1876 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 116.441 -19.186 0.256 -1.675 2.212 –
Hunt & Reffert 2024 116.435 -19.188 0.245 -1.648 2.201 –
Cavallo et al. 2024 116.403 -19.166 0.246 – – –
Hunt & Reffert 2023 116.435 -19.188 0.245 -1.648 2.201 –

💡 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– 4.03 0.61 1.44 232 0.100 174 – –
Hunt & Reffert 2024 4.03 0.61 1.44 232 – 174(1) – –
Cavallo et al. 2024 3.56 0.56 – 417 0.100 – – –
Hunt & Reffert 2023 4.03 0.61 1.44 232 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1414 56.0 116.44 -19.17 0.24 -1.72 2.24 – 0.12

💡 Note: The % column shows the percentage of members that HSC 1876 shares with each listed object.

Visualization

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