CWNU 2452

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0.42 UTI
0.4
CN
0.83
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.83 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2452 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 149.887 -58.714 0.196 -5.304 3.441 18.468
Hunt & Reffert 2024 149.888 -58.713 0.194 -5.311 3.446 12.565
Cavallo et al. 2024 149.873 -58.72 0.195 – – –
Hunt & Reffert 2023 149.888 -58.713 0.194 -5.311 3.446 12.565
He et al. 2023 149.892 -58.718 0.205 -5.296 3.456 8.84

💡 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 – – – – – 963* – –
Cavallo et al. 2024 4.13 2.94 – 263 -0.250 – – –
Hunt & Reffert 2023 4.86 2.75 2.20 106 – – – –
He et al. 2023 3.98 2.10 – 562 – – – –

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

Visualization

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