CWNU 360

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0.53 UTI
0.4
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.4 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 360 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 metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Metal-rich 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 – 234.506 -57.091 0.386 -3.604 -2.669 14.079
Hunt & Reffert 2024 234.538 -57.094 0.391 -3.563 -2.676 15.57
Cavallo et al. 2024 234.517 -57.088 0.386 – – –
Hunt & Reffert 2023 234.538 -57.094 0.391 -3.563 -2.676 15.57
He et al. 2022 234.53 -57.082 0.39 -3.6 -2.68 –

💡 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 – – – – – 568* – –
Cavallo et al. 2024 2.61 3.69 – 107 0.830 – – –
Hunt & Reffert 2023 2.38 4.38 2.02 70 – – – –
He et al. 2022 2.09 3.48 – 501 0.968 – – –

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

Visualization

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