CWNU 1284

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0.52 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 12.4 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1284 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young 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 P93, along with CWNU_2708.

Cavallo et al. (2024)
Bronze 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– 272.14 -21.076 0.364 -1.242 -2.596 -28.968
Hunt & Reffert 2024 272.149 -21.071 0.366 -1.232 -2.592 -19.625
Cavallo et al. 2024 272.126 -21.08 0.366 – – –
Hunt & Reffert 2023 272.149 -21.071 0.366 -1.232 -2.592 -19.625
He et al. 2023 272.14 -21.084 0.366 -1.246 -2.594 -29.4

💡 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– 2.75 4.19 2.55 87 0.750 683 – –
Hunt & Reffert 2024 – – – – – 683(1) – –
Cavallo et al. 2024 2.95 4.19 – 87 0.750 – – –
Hunt & Reffert 2023 2.44 4.01 2.55 86 – – – –
He et al. 2023 2.75 4.60 – 316 – – – –

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

Visualization

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