CWNU 2468

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0.52 UTI
0.36
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.36 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 2468 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 near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Near-solar metallicity Very young

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 – 242.017 -53.136 0.301 -2.649 -3.906 24.179
Hunt & Reffert 2024 242.017 -53.148 0.3 -2.653 -3.906 1.677
Cavallo et al. 2024 242.03 -53.15 0.301 – – –
Hunt & Reffert 2023 242.017 -53.148 0.3 -2.653 -3.906 1.677
He et al. 2023 242.014 -53.152 0.31 -2.664 -3.908 20.35

💡 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 – – – – – 955* – –
Cavallo et al. 2024 3.72 3.90 – 18 -0.310 – – –
Hunt & Reffert 2023 3.02 4.33 0.97 18 – – – –
He et al. 2023 3.47 4.60 – 5 – – – –

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

Visualization

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