CWNU 2590

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0.57 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2590 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 276.34 -12.137 0.344 -0.958 -3.607 22.495
Hunt & Reffert 2024 276.338 -12.125 0.336 -0.975 -3.6 24.835
Cavallo et al. 2024 276.346 -12.147 0.337 – – –
Hunt & Reffert 2023 276.338 -12.125 0.336 -0.975 -3.6 24.835
He et al. 2023 276.346 -12.132 0.352 -0.947 -3.598 23.35

💡 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 – – – – – 1849* – –
Cavallo et al. 2024 3.06 4.19 – 251 -0.050 – – –
Hunt & Reffert 2023 2.64 4.22 3.02 149 – – – –
He et al. 2023 2.45 3.80 – 708 – – – –

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

Visualization

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