CWNU 1230

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0.51 UTI
0.43
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 38.0 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1230 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Wood 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– 336.657 61.276 1.286 -0.249 -2.844 -28.544
Hunt & Reffert 2024 336.619 61.25 1.278 -0.198 -2.829 -28.539
Cavallo et al. 2024 336.562 61.28 1.294 – – –
Hunt & Reffert 2023 336.619 61.25 1.278 -0.198 -2.829 -28.539
He et al. 2022 336.653 61.235 1.3 -0.214 -2.788 –

💡 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– 0.95 2.95 2.32 37 0.390 96 – –
Hunt & Reffert 2024 – – – – – 96(1) – –
Cavallo et al. 2024 1.15 2.57 – 2512 0.390 – – –
Hunt & Reffert 2023 0.75 4.66 2.32 37 – – – –
He et al. 2022 – 2.95 – 2 – – – –

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

Visualization

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