CWNU 1362

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0.55 UTI
0.49
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.49 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 1362 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High 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 – 228.876 -59.177 0.316 -4.324 -4.213 -147.628
Hunt & Reffert 2024 228.877 -59.177 0.316 -4.352 -4.2 -109.251
Cavallo et al. 2024 228.861 -59.178 0.318 – – –
Hunt & Reffert 2023 228.877 -59.177 0.316 -4.352 -4.2 -109.251
He et al. 2023 228.863 -59.17 0.316 -4.327 -4.208 –

💡 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 – – – – – 969* – –
Cavallo et al. 2024 2.39 3.49 – 135 0.050 – – –
Hunt & Reffert 2023 2.82 3.44 1.92 71 – – – –
He et al. 2023 2.82 3.55 – 141 – – – –

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

Visualization

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