HSC 2778

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0.07 UTI
0.0
CN
0.09
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2778 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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.

Palma et al. (2025)
Part of multiple system G165, along with HSC_2785, NGC_6134, NGC_6193, Theia_1643, NGC_6204 and CWNU_1842.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 250.597 -50.773 0.836 -0.368 -0.675 –
Hunt & Reffert 2024 250.651 -50.763 0.837 -0.374 -0.73 –
Hunt & Reffert 2023 250.651 -50.763 0.837 -0.374 -0.73 –

💡 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– 1.13 2.09 1.29 156 – 77 – –
Hunt & Reffert 2024 – – – – – 77(1) – –
Hunt & Reffert 2023 1.13 2.09 1.29 156 – – – –

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

Visualization

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