CWNU 2558

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0.45 UTI
0.45
CN
0.46
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2558 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

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 99999– 101.229 0.888 0.673 -1.492 0.797 -20.599
Zhang et al. 2024 101.249 0.864 – – – –
Hunt & Reffert 2024 101.249 0.864 0.667 -1.479 0.786 -20.635
Cavallo et al. 2024 101.262 0.903 0.667 – – –
Hunt & Reffert 2023 101.249 0.864 0.667 -1.479 0.786 -20.635
He et al. 2023 101.29 0.889 0.673 -1.479 0.797 38.93

💡 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] Bfrac BSS
UCC 99999– 1.45 0.88 1.1 209 -0.029 209 – –
Zhang et al. 2024 – – – – -0.138(1) – – –
Hunt & Reffert 2024 – – – – – 209(1) – –
Cavallo et al. 2024 1.47 0.84 – 209 0.080 – – –
Hunt & Reffert 2023 1.41 0.88 1.10 78 – – – –
He et al. 2023 1.45 1.05 – 501 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14140 55.6 101.23 0.95 0.67 -1.49 0.8 -20.6 0.0

💡 Note: The % column shows the percentage of members that CWNU 2558 shares with each listed object.

Visualization

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