CWNU 1287

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0.34 UTI
0.39
CN
0.18
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1287 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young 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– 325.096 50.469 0.23 -3.473 -3.681 22.025
Hunt & Reffert 2024 325.099 50.525 0.231 -3.461 -3.67 22.026
Cavallo et al. 2024 325.078 50.401 0.226 – – –
Hunt & Reffert 2023 325.099 50.525 0.231 -3.461 -3.67 22.026
He et al. 2023 325.074 50.471 0.227 -3.449 -3.699 -86.06

💡 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– 4.05 2.28 2.34 10 0.490 988 – –
Hunt & Reffert 2024 – – – – – 988(1) – –
Cavallo et al. 2024 3.25 2.27 – 30 0.490 – – –
Hunt & Reffert 2023 4.05 2.28 2.34 10 – – – –
He et al. 2023 4.68 2.70 – 4 – – – –

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

Visualization

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