CWNU 2621

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0.19 UTI
0.0
CN
0.21
Cdens
0.75
CC3
0.06
Clit
0.88
Cdup
Core radius and density 1.3 [pc], 1.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

â„šī¸
CWNU 2621 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very high extinction. It is catalogued as a massive, 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.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.17 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.17 (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– 259.774 -42.356 0.262 -0.972 -3.177 -78.012
Hunt & Reffert 2024 259.784 -42.356 0.257 -0.945 -3.167 -60.965
Cavallo et al. 2024 259.758 -42.36 0.255 – – –
Hunt & Reffert 2023 259.784 -42.356 0.257 -0.945 -3.167 -60.965
He et al. 2023 259.772 -42.362 0.272 -0.927 -3.178 -69.45

💡 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– 3.3 5.135 2.63 142 0.470 1518 – –
Hunt & Reffert 2024 3.30 5.17 2.63 101 – 1518(1) – –
Cavallo et al. 2024 3.56 4.32 – 182 0.470 – – –
Hunt & Reffert 2023 3.30 5.17 2.63 101 – – – –
He et al. 2023 3.02 5.10 – 562 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVVX CL056 12.0 259.49 -42.23 0.27 -0.99 -3.15 -52.87 0.05

💡 Note: The % column shows the percentage of members that CWNU 2621 shares with each listed object.

Visualization

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