CWNU 2522

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0.29 UTI
0.0
CN
0.21
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2522 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 163.601 -57.317 0.377 -6.714 2.658 –
Hunt & Reffert 2024 163.533 -57.4 0.371 -6.692 2.638 –
Cavallo et al. 2024 163.582 -57.384 0.371 – – –
Hunt & Reffert 2023 163.533 -57.4 0.371 -6.692 2.638 –
He et al. 2023 163.634 -57.328 0.381 -6.701 2.657 –

💡 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 – – – – – 93* – –
Cavallo et al. 2024 3.13 1.23 – 22 -0.150 – – –
Hunt & Reffert 2023 2.48 0.82 0.44 93 – – – –
He et al. 2023 2.45 1.35 – 40 – – – –

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

Visualization

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