HSC 290

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0.27 UTI
0.66
CN
0.04
Cdens
0.62
CC3
0.03
Clit
0.98
Cdup
Core radius and density 6.0 [pc], 0.2 [pc-2]
  • CN 0.66 Moderately populated
  • Cdens 0.04 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 0.98 Unique

Overview

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HSC 290 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as an extremely massive, near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.04 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.04 (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– 278.975 -2.338 0.144 -2.538 -5.41 40.949
Hunt & Reffert 2024 278.966 -2.335 0.143 -2.586 -5.448 45.177
Cavallo et al. 2024 278.957 -2.37 0.147 – – –
Hunt & Reffert 2023 278.966 -2.335 0.143 -2.586 -5.448 45.177

💡 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– 5.23 5.2 2.99 1972 -0.100 10123 – –
Hunt & Reffert 2024 5.23 5.20 2.99 1971 – 10123(1) – –
Cavallo et al. 2024 5.40 3.89 – 2570 -0.100 – – –
Hunt & Reffert 2023 5.23 5.20 2.99 1972 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 905 2.4 278.97 -2.53 0.16 -2.89 -5.53 -6.43 0.09

💡 Note: The % column shows the percentage of members that HSC 290 shares with each listed object.

Visualization

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