CWNU 2765

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0.64 UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.4 [N/pc2]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2765 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, 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.

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– 261.156 -38.572 0.364 -0.315 -2.719 -33.831
Hunt & Reffert 2024 261.153 -38.581 0.353 -0.309 -2.726 -25.906
Cavallo et al. 2024 261.164 -38.583 0.354 – – –
Hunt & Reffert 2023 261.153 -38.581 0.353 -0.309 -2.726 -25.906
He et al. 2023 261.144 -38.58 0.366 -0.324 -2.724 -37.17

💡 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– 2.34 4.21 2.69 214 -0.040 1603 – –
Hunt & Reffert 2024 – – – – – 1603(1) – –
Cavallo et al. 2024 1.97 4.25 – 214 -0.040 – – –
Hunt & Reffert 2023 2.49 4.21 2.69 97 – – – –
He et al. 2023 2.34 2.75 – 1413 – – – –

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

Visualization

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