CWNU 2718

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0.59 UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 38.6 [N/pc2]
  • CN 0.72 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 2718 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 metal-poor, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P113, along with Dias_6.

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– 277.002 -12.165 0.335 -0.516 -3.519 40.296
Hunt & Reffert 2024 277.007 -12.163 0.325 -0.529 -3.533 40.265
Cavallo et al. 2024 276.999 -12.172 0.323 – – –
Hunt & Reffert 2023 277.007 -12.163 0.325 -0.529 -3.533 40.265
He et al. 2023 277.002 -12.166 0.338 -0.527 -3.52 41.27

💡 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– 2.62 4.3 2.53 99 -0.680 990 – –
Hunt & Reffert 2024 – – – – – 990(1) – –
Cavallo et al. 2024 2.62 4.45 – 66 -0.680 – – –
Hunt & Reffert 2023 2.68 4.04 2.53 99 – – – –
He et al. 2023 2.45 4.30 – 398 – – – –

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

Visualization

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