HSC 2019

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0.20 UTI
0.46
CN
0.11
Cdens
0.38
CC3
0.03
Clit
1.0
Cdup
Core radius and density 3.0 [pc], 0.6 [pc-2]
  • CN 0.46 Poorly populated
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2019 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a 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)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 121.107 -33.985 0.29 -3.294 4.866 –
Hunt & Reffert 2024 121.078 -33.962 0.292 -3.316 4.848 –
Cavallo et al. 2024 121.125 -33.973 0.293 – – –
Hunt & Reffert 2023 121.078 -33.962 0.292 -3.316 4.848 –

💡 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– 3.15 1.91 0.68 180 0.290 331 – –
Hunt & Reffert 2024 3.15 1.91 0.68 180 – 331(1) – –
Cavallo et al. 2024 2.86 2.11 – 257 0.290 – – –
Hunt & Reffert 2023 3.15 1.91 0.68 179 – – – –

(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 3088 95.7 121.12 -33.99 0.29 -3.31 4.86 – 0.05

💡 Note: The % column shows the percentage of members that HSC 2019 shares with each listed object.

Visualization

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