CWNU 2907

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0.11 UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2907 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Palma et al. (2025)
Classified as optical pair P366, along with UBC_482.

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– 129.934 -45.532 0.467 -5.812 4.585 –
Hunt & Reffert 2024 129.948 -45.521 0.46 -5.803 4.607 –
Cavallo et al. 2024 129.892 -45.555 0.46 – – –
Hunt & Reffert 2023 129.948 -45.521 0.46 -5.803 4.607 –
He et al. 2023 129.942 -45.546 0.451 -5.812 4.589 –

💡 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– 2.105 1.51 0.54 84 -0.300 117 – –
Hunt & Reffert 2024 2.02 1.51 0.54 148 – 117(1) – –
Cavallo et al. 2024 2.22 2.15 – 19 -0.300 – – –
Hunt & Reffert 2023 2.02 1.51 0.54 148 – – – –
He et al. 2023 2.19 1.10 – 11 – – – –

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

Visualization

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