CWNU 62

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0.39 UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Stellar density (N50/rad) 8.7 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 62 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied in the literature.

Palma et al. (2025)
Part of multiple system G57, along with CWNU_2606 and CWNU_2714.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.11 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.11 (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– 256.715 -41.555 0.641 1.202 -2.022 5.83
Hunt & Reffert 2024 256.701 -41.565 0.632 1.203 -1.996 -18.327
Cavallo et al. 2024 256.708 -41.594 0.633 – – –
Hunt & Reffert 2023 256.701 -41.565 0.632 1.203 -1.996 -18.327
He et al. 2022 256.7 -41.589 0.62 1.23 -2.02 –

💡 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– 1.5 3.24 2.42 68 0.203 390 – –
Hunt & Reffert 2024 – – – – – 390(1) – –
Cavallo et al. 2024 1.45 2.79 – 389 0.510 – – –
Hunt & Reffert 2023 1.50 3.24 2.42 68 – – – –
He et al. 2022 1.58 3.80 – 25 -0.103 – – –

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

Visualization

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