CWNU 1851

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0.24 UTI
0.0
CN
0.33
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.33 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1851 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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 Moderate extinction Metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 254.419 -41.457 0.604 -0.52 -0.051 -44.68
Hunt & Reffert 2024 254.405 -41.466 0.616 -0.508 -0.075 -44.678
Cavallo et al. 2024 254.457 -41.429 0.611 – – –
Hunt & Reffert 2023 254.405 -41.466 0.616 -0.508 -0.075 -44.678
He et al. 2023 254.424 -41.458 0.608 -0.498 -0.042 –

💡 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 – – – – – 121* – –
Cavallo et al. 2024 1.58 1.92 – 191 -0.800 – – –
Hunt & Reffert 2023 1.57 1.76 1.03 102 – – – –
He et al. 2023 1.55 1.95 – 89 – – – –

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

Visualization

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