HSC 455

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0.15 UTI
0.26
CN
0.1
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.4 [pc], 0.5 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 455 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.90 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.90 (50th percentile), true positive (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 287.124 23.378 1.062 0.287 -0.517 -10.402
Zhang et al. 2024 287.108 23.385 – – – –
Hunt & Reffert 2024 287.108 23.385 1.068 0.319 -0.511 -6.078
Cavallo et al. 2024 287.232 23.318 1.062 – – –
Hunt & Reffert 2023 287.108 23.385 1.068 0.319 -0.511 -6.078

💡 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– 0.89 1.51 0.38 97 -0.002 62 – –
Zhang et al. 2024 – – – – -0.063(1) – – –
Hunt & Reffert 2024 0.89 1.51 0.38 97 – 62(1) – –
Cavallo et al. 2024 0.96 1.76 – 316 0.060 – – –
Hunt & Reffert 2023 0.89 1.51 0.38 97 – – – –

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

Visualization

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