CWNU 1422

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0.18 UTI
0.3
CN
0.22
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 1.1 [pc-2]
  • CN 0.3 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1422 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (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.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P307, along with FSR_0665.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 62.824 51.232 0.331 -0.391 -0.663 –
Hunt & Reffert 2024 62.839 51.217 0.324 -0.39 -0.66 –
Cavallo et al. 2024 62.848 51.254 0.329 – – –
Hunt & Reffert 2023 62.839 51.217 0.324 -0.39 -0.66 –
He et al. 2023 62.834 51.236 0.349 -0.383 -0.664 –

💡 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– 2.8 2.93 1.32 62 0.560 333 – –
Hunt & Reffert 2024 2.80 2.93 1.32 62 – 333(1) – –
Cavallo et al. 2024 3.42 2.85 – 59 0.560 – – –
Hunt & Reffert 2023 2.80 2.93 1.32 62 – – – –
He et al. 2023 2.51 2.95 – 398 – – – –

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

Visualization

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