CWNU 367

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0.14 UTI
0.0
CN
0.08
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.8 [pc], 0.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 367 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied 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 class: 0.38 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.38 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 274.124 -12.687 0.669 -1.137 -0.594 –
Hunt & Reffert 2024 274.118 -12.718 0.708 -1.185 -0.636 18.823
Cavallo et al. 2024 274.123 -12.698 0.705 – – –
Hunt & Reffert 2023 274.118 -12.718 0.708 -1.185 -0.636 18.823
He et al. 2022 274.111 -12.72 0.69 -1.06 -0.58 –

💡 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– 1.365 1.535 1.69 368 -0.370 127 – –
Hunt & Reffert 2024 1.37 1.50 1.69 330 – 127(1) – –
Cavallo et al. 2024 1.36 1.57 – 407 0.140 – – –
Hunt & Reffert 2023 1.37 1.50 1.69 330 – – – –
He et al. 2022 1.15 2.09 – 1259 -0.881 – – –

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

Visualization

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