CWNU 2622

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0.48 UTI
0.3
CN
0.87
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.87 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2622 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 258.267 -41.786 0.442 -1.494 -4.024 -34.003
Hunt & Reffert 2024 258.262 -41.799 0.439 -1.478 -4.02 –
Cavallo et al. 2024 258.255 -41.786 0.442 – – –
Hunt & Reffert 2023 258.262 -41.799 0.439 -1.478 -4.02 –
He et al. 2023 258.26 -41.778 0.446 -1.491 -3.996 -13.27

💡 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 – – – – – 383* – –
Cavallo et al. 2024 1.99 2.85 – 105 0.220 – – –
Hunt & Reffert 2023 2.06 2.89 1.25 68 – – – –
He et al. 2023 1.95 2.95 – 355 – – – –

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

Visualization

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