CWNU 2616

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0.50 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 18.0 [N/pc2]
  • CN 0.0 Sparse
  • 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 2616 is a sparse, 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 near-solar metallicity, 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– 199.3 -63.892 0.206 -5.878 -0.488 –
Hunt & Reffert 2024 199.298 -63.891 0.204 -5.883 -0.489 –
Cavallo et al. 2024 199.299 -63.884 0.206 – – –
Hunt & Reffert 2023 199.298 -63.891 0.204 -5.883 -0.489 –
He et al. 2023 199.307 -63.893 0.212 -5.878 -0.496 –

💡 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– 4.42 3.13 1.97 52 -0.400 468 – –
Hunt & Reffert 2024 – – – – – 468(1) – –
Cavallo et al. 2024 2.74 3.13 – 71 -0.400 – – –
Hunt & Reffert 2023 4.42 3.08 1.97 52 – – – –
He et al. 2023 4.68 3.70 – 3 – – – –

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

Visualization

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