CWNU 1635

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0.53 UTI
0.42
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 18.7 [N/pc2]
  • CN 0.42 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 1635 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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 99999– 117.93 -32.362 0.31 -3.469 4.934 51.937
Hunt & Reffert 2024 117.931 -32.362 0.312 -3.468 4.902 51.946
Cavallo et al. 2024 117.924 -32.336 0.314 – – –
Hunt & Reffert 2023 117.931 -32.362 0.312 -3.468 4.902 51.946
He et al. 2023 117.936 -32.363 0.297 -3.456 4.94 51.94

💡 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] Bfrac BSS
UCC 99999– 2.81 2.71 1.71 357 -0.460 347 – –
Hunt & Reffert 2024 – – – – – 347(1) – –
Cavallo et al. 2024 2.47 2.71 – 417 -0.460 – – –
Hunt & Reffert 2023 2.81 2.40 1.71 357 – – – –
He et al. 2023 2.88 2.75 – 282 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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