CWNU 2714

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0.56 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.5 [N/pc2]
  • CN 0.55 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 2714 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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)
Part of multiple system G57, along with CWNU_2606 and CWNU_62.

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– 256.927 -42.645 0.621 1.069 -1.811 -35.031
Hunt & Reffert 2024 256.917 -42.649 0.617 1.043 -1.864 -25.466
Cavallo et al. 2024 256.852 -42.676 0.618 – – –
Hunt & Reffert 2023 256.917 -42.649 0.617 1.043 -1.864 -25.466
He et al. 2023 256.91 -42.635 0.622 1.076 -1.803 -26.67

💡 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– 1.51 3.0 2.11 78 0.810 470 – –
Hunt & Reffert 2024 – – – – – 470(1) – –
Cavallo et al. 2024 1.79 3.02 – 78 0.810 – – –
Hunt & Reffert 2023 1.51 2.92 2.11 55 – – – –
He et al. 2023 1.51 3.00 – 447 – – – –

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

Visualization

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