CWNU 2410

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0.52 UTI
0.58
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.58 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 2410 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 183.07 -61.973 0.21 -7.157 0.714 -24.957
Hunt & Reffert 2024 183.083 -61.969 0.221 -7.158 0.701 -28.695
Cavallo et al. 2024 183.081 -61.976 0.217 – – –
Hunt & Reffert 2023 183.083 -61.969 0.221 -7.158 0.701 -28.695
He et al. 2023 183.083 -61.979 0.22 -7.151 0.727 -24.96

💡 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 – – – – – 1239* – –
Cavallo et al. 2024 4.04 3.78 – 60 0.360 – – –
Hunt & Reffert 2023 4.05 3.51 2.59 56 – – – –
He et al. 2023 3.63 3.80 – 63 – – – –

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

Visualization

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