CWNU 2556

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0.41 UTI
0.32
CN
0.62
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.62 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2556 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a large distance, below 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.
Very distant 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 – 353.802 56.7 0.181 -1.94 -1.083 –
Hunt & Reffert 2024 353.789 56.708 0.176 -1.94 -1.072 –
Cavallo et al. 2024 353.751 56.691 0.176 – – –
Hunt & Reffert 2023 353.789 56.708 0.176 -1.94 -1.072 –
He et al. 2023 353.804 56.708 0.188 -1.947 -1.084 –

💡 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 – – – – – 210* – –
Cavallo et al. 2024 4.19 1.98 – 427 -0.230 – – –
Hunt & Reffert 2023 5.17 1.89 2.21 314 – – – –
He et al. 2023 6.03 2.25 – 501 – – – –

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

Visualization

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