CWNU 1273

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0.39 UTI
0.45
CN
0.49
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.5 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1273 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a 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.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P92, along with HSC_1893.

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– 115.046 -21.968 0.36 -3.217 3.146 36.91
Hunt & Reffert 2024 115.049 -22.005 0.361 -3.21 3.135 24.112
Cavallo et al. 2024 115.044 -21.976 0.359 – – –
Hunt & Reffert 2023 115.049 -22.005 0.361 -3.21 3.135 24.112
He et al. 2023 115.068 -21.97 0.363 -3.228 3.154 –

💡 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– 2.43 0.99 1.43 163 0.320 161 – –
Hunt & Reffert 2024 – – – – – 161(1) – –
Cavallo et al. 2024 2.43 0.99 – 204 0.320 – – –
Hunt & Reffert 2023 2.43 0.90 1.43 163 – – – –
He et al. 2023 2.45 1.25 – 35 – – – –

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

Visualization

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