CWNU 1416

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0.16 UTI
0.26
CN
0.01
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 7.2 [pc], 0.06 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.01 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1416 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a very 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.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.18 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.18 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 351.193 62.664 0.313 -3.921 -1.691 -86.166
Hunt & Reffert 2024 351.211 62.371 0.305 -3.932 -1.694 –
Cavallo et al. 2024 351.215 62.719 0.304 – – –
Hunt & Reffert 2023 351.211 62.371 0.305 -3.932 -1.694 –
He et al. 2023 351.396 62.941 0.323 -3.961 -1.621 -94.07

💡 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– 2.93 3.08 2.51 45 1.030 222 – –
Hunt & Reffert 2024 2.93 3.08 2.51 25 – 222(1) – –
Cavallo et al. 2024 3.52 2.71 – 65 1.030 – – –
Hunt & Reffert 2023 2.93 3.08 2.51 25 – – – –
He et al. 2023 2.75 3.55 – 282 – – – –

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

Visualization

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