CWNU 1355

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0.24 UTI
0.34
CN
0.16
Cdens
0.5
CC3
0.1
Clit
1.0
Cdup
Core radius and density 0.6 [pc], 0.8 [pc-2]
  • CN 0.34 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1355 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close 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 and metallicity parameters (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: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 96.065 21.074 0.606 -0.809 -4.071 –
Zhang et al. 2024 96.059 21.098 – – – –
Hunt & Reffert 2024 96.059 21.098 0.607 -0.778 -4.074 –
Cavallo et al. 2024 96.054 21.057 0.612 – – –
Hunt & Reffert 2023 96.059 21.098 0.607 -0.778 -4.074 –
He et al. 2023 96.088 21.057 0.612 -0.811 -4.056 –

💡 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– 1.59 0.89 0.85 299 0.121 174 – –
Zhang et al. 2024 – – – – -0.098(1) – – –
Hunt & Reffert 2024 1.52 0.81 0.85 299 – 174(1) – –
Cavallo et al. 2024 1.99 0.97 – 324 0.340 – – –
Hunt & Reffert 2023 1.52 0.81 0.85 299 – – – –
He et al. 2023 1.66 1.05 – 40 – – – –

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

Visualization

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