CWNU 2921

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0.19 UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2921 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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 Low extinction Near-solar metallicity 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 – 114.167 -33.594 0.449 -3.519 3.827 –
Hunt & Reffert 2024 114.199 -33.571 0.442 -3.499 3.801 –
Cavallo et al. 2024 114.089 -33.614 0.451 – – –
Hunt & Reffert 2023 114.199 -33.571 0.442 -3.499 3.801 –
He et al. 2023 114.141 -33.604 0.446 -3.537 3.841 –

💡 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 – – – – – 70* – –
Cavallo et al. 2024 2.16 0.62 – 200 0.010 – – –
Hunt & Reffert 2023 2.09 0.95 1.58 177 – – – –
He et al. 2023 2.24 1.35 – 18 – – – –

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

Visualization

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