HSC 2878

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0.18 UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2878 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~12.06 kpc) differs significantly from the median photometric distance (~7.67 kpc).

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)
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 99999– 256.087 -37.019 0.083 -3.861 -5.101 20.227
Hu & Soubiran 2025 256.079 -37.035 – – – –
Hunt & Reffert 2024 256.102 -37.011 0.094 -3.837 -5.103 -95.69
Cavallo et al. 2024 256.079 -37.035 0.094 – – –
Hunt & Reffert 2023 256.102 -37.011 0.094 -3.837 -5.103 -95.69

💡 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– 7.675 4.06 2.41 2297 -0.220 4280 – –
Hu & Soubiran 2025 – – – – -0.410(5) – – –
Hunt & Reffert 2024 – – – – – 4280(1) – –
Cavallo et al. 2024 7.01 3.25 – 3467 -0.030 – – –
Hunt & Reffert 2023 8.34 4.87 2.41 1127 – – – –

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

Visualization

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