CWNU 2583

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0.28 UTI
0.31
CN
0.21
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.3 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2583 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High 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 – 326.747 56.935 0.447 -4.508 -3.518 4.931
Hunt & Reffert 2024 326.696 56.884 0.44 -4.498 -3.513 5.007
Cavallo et al. 2024 326.803 57.025 0.444 – – –
Hunt & Reffert 2023 326.696 56.884 0.44 -4.498 -3.513 5.007
He et al. 2023 326.712 56.987 0.446 -4.514 -3.503 –

💡 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 – – – – – 324* – –
Cavallo et al. 2024 2.11 3.09 – 32 0.350 – – –
Hunt & Reffert 2023 2.14 3.06 1.74 26 – – – –
He et al. 2023 2.04 3.50 – 18 – – – –

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

Visualization

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