CWNU 1333

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0.48 UTI
0.46
CN
0.95
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 0.95 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1333 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive 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 – 220.016 -61.302 0.234 -4.507 -3.124 -31.058
Hunt & Reffert 2024 220.006 -61.29 0.238 -4.486 -3.117 -46.834
Cavallo et al. 2024 220.012 -61.297 0.236 – – –
Hunt & Reffert 2023 220.006 -61.29 0.238 -4.486 -3.117 -46.834
He et al. 2023 220.01 -61.3 0.254 -4.533 -3.12 -15.27

💡 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 – – – – – 1289* – –
Cavallo et al. 2024 3.24 4.34 – 490 0.290 – – –
Hunt & Reffert 2023 3.55 4.23 2.19 191 – – – –
He et al. 2023 3.31 3.90 – 708 – – – –

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

Visualization

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