CWNU 1560

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0.54 UTI
0.45
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 11.4 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1560 is a poorly 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-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Part of multiple system G39, along with CWNU_2792, HSC_2678 and CWNU_1528.

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– 228.006 -58.722 0.41 -4.148 -4.183 157.482
Hunt & Reffert 2024 227.994 -58.718 0.409 -4.154 -4.151 157.513
Cavallo et al. 2024 228.027 -58.706 0.41 – – –
Hunt & Reffert 2023 227.994 -58.718 0.409 -4.154 -4.151 157.513
He et al. 2023 228.029 -58.714 0.41 -4.133 -4.183 –

💡 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– 2.21 4.04 2.04 158 0.530 607 – –
Hunt & Reffert 2024 – – – – – 607(1) – –
Cavallo et al. 2024 2.42 3.63 – 209 0.530 – – –
Hunt & Reffert 2023 2.21 4.04 2.04 57 – – – –
He et al. 2023 2.14 4.05 – 158 – – – –

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

Visualization

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