CWNU 279

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0.13 UTI
0.0
CN
0.15
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.8 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 279 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 absorption and metallicity parameters (see Parameters). It is rarely studied 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 103.831 -2.134 0.537 -1.416 1.093 80.19
Hunt & Reffert 2024 103.827 -2.132 0.55 -1.401 1.123 29.007
Cavallo et al. 2024 103.83 -2.151 0.554 – – –
Hunt & Reffert 2023 103.827 -2.132 0.55 -1.401 1.123 29.007
He et al. 2022 103.839 -2.151 0.53 -1.42 1.09 –

💡 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– 1.725 0.29 0.78 111 0.231 91 – –
Hunt & Reffert 2024 1.74 0.29 0.78 111 – 91(1) – –
Cavallo et al. 2024 1.71 0.04 – 219 0.740 – – –
Hunt & Reffert 2023 1.74 0.29 0.78 111 – – – –
He et al. 2022 1.48 0.51 – 63 -0.279 – – –

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

Visualization

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