CWNU 1334

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0.13 UTI
0.0
CN
0.09
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.6 [pc], 0.5 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1334 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 100.528 16.448 0.356 -0.729 -1.048 32.103
Zhang et al. 2024 100.581 16.433 – – – –
Hunt & Reffert 2024 100.581 16.433 0.371 -0.727 -1.032 32.1
Cavallo et al. 2024 100.538 16.439 0.368 – – –
Hunt & Reffert 2023 100.581 16.433 0.371 -0.727 -1.032 32.1
He et al. 2023 100.561 16.467 0.35 -0.727 -1.059 –

💡 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– 2.48 0.93 0.98 180 -0.340 166 – –
Zhang et al. 2024 – – – – -0.380(1) – – –
Hunt & Reffert 2024 2.48 0.91 0.98 180 – 166(1) – –
Cavallo et al. 2024 2.62 1.47 – 23 -0.300 – – –
Hunt & Reffert 2023 2.48 0.91 0.98 180 – – – –
He et al. 2023 2.45 0.95 – 224 – – – –

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

Visualization

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