CWNU 1074

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0.20 UTI
0.0
CN
0.13
Cdens
0.5
CC3
0.19
Clit
1.0
Cdup
Core radius and density 2.6 [pc], 0.6 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1074 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (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: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 295.836 6.335 1.347 0.545 -2.003 -8.005
Swiggum et al. 2024 295.903 6.413 1.338 0.355 -2.036 -10.58
Hunt & Reffert 2024 295.903 6.413 1.338 0.355 -2.036 -8.561
Cavallo et al. 2024 295.442 5.261 1.343 – – –
Hunt & Reffert 2023 295.903 6.413 1.338 0.355 -2.036 -8.561
He et al. 2022 295.892 6.445 1.334 0.574 -1.961 –

💡 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– 0.72 0.705 0.8 36 -0.040 380 – –
Swiggum et al. 2024 0.73 – – 36 – 661 – –
Hunt & Reffert 2024 0.71 0.63 0.80 36 – 99(1) – –
Cavallo et al. 2024 0.76 0.77 – 29 -0.040 – – –
Hunt & Reffert 2023 0.71 0.64 0.80 36 – – – –
He et al. 2022 – 0.90 – 35 – – – –

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

Visualization

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