CWNU 1093

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0.33 UTI
0.35
CN
0.44
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 25.4 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1093 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 117.18 20.2 1.842 -6.881 -4.278 18.631
Zhang et al. 2024 117.26 20.179 – – – –
Cavallo et al. 2024 116.827 20.426 1.812 – – –
Hunt & Reffert 2023 117.26 20.179 1.799 -6.956 -4.375 16.622
He et al. 2022 117.061 20.281 1.844 -6.906 -4.299 –

💡 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
Zhang et al. 2024 – – – – -0.101* – – –
Cavallo et al. 2024 0.55 0.32 – 251 0.170 – – –
Hunt & Reffert 2023 0.53 0.09 0.65 243 – – – –
He et al. 2022 – 0.05 – 89 – – – –

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

Visualization

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