CWNU 2485

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0.50 UTI
0.5
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.6 [N/pc2]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2485 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (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– 242.496 -52.733 0.419 -1.233 -2.719 -16.03
Hunt & Reffert 2024 242.509 -52.744 0.417 -1.243 -2.716 –
Cavallo et al. 2024 242.512 -52.712 0.415 – – –
Hunt & Reffert 2023 242.509 -52.744 0.417 -1.243 -2.716 –
He et al. 2023 242.496 -52.745 0.423 -1.209 -2.711 -16.03

💡 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– 2.19 2.55 1.93 32 -0.630 242 – –
Hunt & Reffert 2024 – – – – – 242(1) – –
Cavallo et al. 2024 1.60 2.79 – 32 -0.630 – – –
Hunt & Reffert 2023 2.20 2.33 1.93 61 – – – –
He et al. 2023 2.19 2.55 – 22 – – – –

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

Visualization

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