CWNU 2366

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0.50 UTI
0.5
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.5 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 2366 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, 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)
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 – 313.676 47.668 0.215 -2.784 -3.605 -37.225
Hunt & Reffert 2024 313.675 47.673 0.21 -2.794 -3.591 -36.974
Cavallo et al. 2024 313.675 47.682 0.219 – – –
Hunt & Reffert 2023 313.675 47.673 0.21 -2.794 -3.591 -36.974
He et al. 2023 313.671 47.686 0.224 -2.784 -3.609 -36.46

💡 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 – – – – – 1110* – –
Cavallo et al. 2024 3.80 3.75 – 380 -0.480 – – –
Hunt & Reffert 2023 4.13 3.66 2.68 229 – – – –
He et al. 2023 4.37 4.05 – 200 – – – –

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

Visualization

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