CWNU 488

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0.38 UTI
0.34
CN
0.6
Cdens
0.75
CC3
0.1
Clit
1.0
Cdup
Core radius and density 0.7 [pc], 3.0 [pc-2]
  • CN 0.34 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 488 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.52 kpc) differs significantly from the median photometric distance (~3.72 kpc).

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 77 along with Ruprecht_138.

Palma et al. (2025)
Classified as genetic pair P207, along with Ruprecht_138.

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.88 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.88 (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– 269.571 -25.255 0.397 0.307 -1.416 –
Hunt & Reffert 2024 269.568 -25.258 0.392 0.291 -1.422 –
Cavallo et al. 2024 269.57 -25.265 0.391 – – –
Hunt & Reffert 2023 269.568 -25.258 0.392 0.291 -1.422 –
He et al. 2022 269.574 -25.272 0.38 0.31 -1.42 –

💡 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– 3.72 2.1 2.0 46 -0.863 397 – –
Liu et al. 2025 5.37 0.78 – 15 – – – –
Hunt & Reffert 2024 2.29 2.10 2.00 120 – 397(1) – –
Cavallo et al. 2024 5.11 2.81 – 46 -2.020 – – –
Hunt & Reffert 2023 2.29 2.10 2.00 120 – – – –
He et al. 2022 3.72 3.42 – 5 0.295 – – –

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

Visualization

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