CWNU 2459

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0.50 UTI
0.28
CN
0.72
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2459 is a poorly populated, moderately dense object of very high 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.
Distant Moderate extinction Metal-poor Young

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 – 273.035 -19.184 0.323 -0.75 -2.059 22.63
Hunt & Reffert 2024 273.036 -19.18 0.324 -0.752 -2.065 -87.788
Cavallo et al. 2024 273.029 -19.18 0.324 – – –
Hunt & Reffert 2023 273.036 -19.18 0.324 -0.752 -2.065 -87.788
He et al. 2023 273.036 -19.173 0.323 -0.737 -2.08 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 354* – –
Cavallo et al. 2024 4.97 1.72 – 78 -0.680 – – –
Hunt & Reffert 2023 3.27 1.83 1.14 55 – – – –
He et al. 2023 2.82 2.15 – 28 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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