CWNU 2698

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0.50 UTI
0.43
CN
0.8
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.0 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 0.8 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2698 is a poorly populated, 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.

Palma et al. (2025)
Classified as optical pair P95, along with CWNU_1308.

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 99999– 276.522 -14.761 0.328 0.003 -1.325 26.562
Hunt & Reffert 2024 276.504 -14.777 0.319 0.007 -1.325 -3.66
Cavallo et al. 2024 276.511 -14.764 0.318 – – –
Hunt & Reffert 2023 276.504 -14.777 0.319 0.007 -1.325 -3.66
He et al. 2023 276.514 -14.769 0.35 0.003 -1.33 25.39

💡 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– 2.4 4.52 2.28 151 0.170 1344 – –
Hunt & Reffert 2024 – – – – – 1344(1) – –
Cavallo et al. 2024 2.20 4.52 – 151 0.170 – – –
Hunt & Reffert 2023 2.80 4.03 2.28 61 – – – –
He et al. 2023 2.40 4.75 – 200 – – – –

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

Visualization

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