CWNU 2103

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0.26 UTI
0.26
CN
0.3
Cdens
0.12
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 10.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.12 Very low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2103 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, above 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.
Relatively close Moderate 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 – 103.217 3.929 0.716 -0.869 -3.647 34.495
Zhang et al. 2024 103.2 3.949 – – – –
Hunt & Reffert 2024 103.2 3.949 0.692 -0.863 -3.634 37.573
Cavallo et al. 2024 103.299 3.803 0.696 – – –
Hunt & Reffert 2023 103.2 3.949 0.692 -0.863 -3.634 37.573
He et al. 2023 103.188 3.971 0.727 -0.865 -3.634 –

💡 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 – – – – 0.017* – – –
Hunt & Reffert 2024 – – – – – 95* – –
Cavallo et al. 2024 1.47 1.43 – 129 0.070 – – –
Hunt & Reffert 2023 1.33 1.14 2.24 212 – – – –
He et al. 2023 1.38 2.10 – 40 – – – –

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

Visualization

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