CWNU 2502

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0.22 UTI
0.0
CN
0.23
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.23 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2502 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (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.

Relatively close High extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 305.468 35.834 0.44 -1.178 -3.89 -33.78
Hunt & Reffert 2024 305.433 35.805 0.447 -1.151 -3.855 -28.449
Cavallo et al. 2024 305.424 35.843 0.445 – – –
Hunt & Reffert 2023 305.433 35.805 0.447 -1.151 -3.855 -28.449
He et al. 2023 305.502 35.867 0.45 -1.169 -3.876 -17.0

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 284* – –
Cavallo et al. 2024 2.34 3.05 – 204 0.570 – – –
Hunt & Reffert 2023 2.11 3.79 2.82 64 – – – –
He et al. 2023 2.00 3.55 – 447 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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