CWNU 260

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0.32 UTI
0.32
CN
0.29
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 21.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 260 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Close Low extinction Low mass Metal-rich 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 – 117.471 -49.692 1.306 -4.712 7.787 16.724
Hunt & Reffert 2024 117.494 -49.718 1.263 -4.738 7.669 15.844
Cavallo et al. 2024 117.762 -49.712 1.276 – – –
Hunt & Reffert 2023 117.494 -49.718 1.263 -4.738 7.669 15.844
He et al. 2022 117.435 -49.658 1.3 -4.68 7.85 15.5

💡 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 – – – – – 43* – –
Cavallo et al. 2024 0.76 0.35 – 166 0.320 – – –
Hunt & Reffert 2023 0.73 0.23 0.95 115 – – – –
He et al. 2022 0.91 0.48 – 79 0.968 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 258 18.8 115.43 -50.08 1.38 -4.52 7.78 16.87 0.15

💡 Note: The % column shows the percentage of members that CWNU 260 shares with each listed object.

Visualization

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