CWNU 110

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0.38 UTI
0.0
CN
0.76
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.76 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 110 is a sparse, dense object of intermediate C3 quality. Its parallax locates it at a relatively 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.
Relatively close Low 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 – 113.844 -15.618 0.745 -3.631 1.808 38.059
Hunt & Reffert 2024 113.874 -15.562 0.706 -3.554 1.809 39.906
Cavallo et al. 2024 113.871 -15.584 0.717 – – –
Hunt & Reffert 2023 113.874 -15.562 0.706 -3.554 1.809 39.906
He et al. 2022 113.853 -15.61 0.72 -3.61 1.82 21.8

💡 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 – – – – – 90* – –
Cavallo et al. 2024 1.34 0.45 – 263 0.030 – – –
Hunt & Reffert 2023 1.28 0.15 0.28 217 – – – –
He et al. 2022 1.62 0.36 – 398 0.916 – – –

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

Visualization

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