CWNU 2750

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0.43 UTI
0.45
CN
0.43
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.43 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2750 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Palma et al. (2025)
Part of multiple system G58, along with CWNU_1685 and UBC_286.

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– 186.963 -61.978 0.462 -5.195 -0.202 –
Hunt & Reffert 2024 186.971 -61.986 0.451 -5.227 -0.209 -54.748
Cavallo et al. 2024 187.082 -61.969 0.449 – – –
Hunt & Reffert 2023 186.971 -61.986 0.451 -5.227 -0.209 -54.748
He et al. 2023 186.973 -61.979 0.457 -5.199 -0.206 –

💡 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– 2.04 1.39 1.88 22 -0.120 272 – –
Hunt & Reffert 2024 – – – – – 272(1) – –
Cavallo et al. 2024 2.06 1.72 – 18 -0.120 – – –
Hunt & Reffert 2023 2.01 1.39 1.88 44 – – – –
He et al. 2023 2.04 1.35 – 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2520 2.2 186.21 -61.79 0.46 -5.3 -0.24 – 0.09

💡 Note: The % column shows the percentage of members that CWNU 2750 shares with each listed object.

Visualization

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