CWNU 2918

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0.26 UTI
0.27
CN
0.26
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2918 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 105.848 -6.952 0.374 -1.184 0.693 –
Hunt & Reffert 2024 105.841 -6.957 0.37 -1.169 0.672 –
Cavallo et al. 2024 105.868 -6.979 0.37 – – –
Hunt & Reffert 2023 105.841 -6.957 0.37 -1.169 0.672 –
He et al. 2023 105.843 -6.894 0.381 -1.182 0.696 –

💡 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 – – – – – 251* – –
Cavallo et al. 2024 2.32 1.11 – 380 -0.050 – – –
Hunt & Reffert 2023 2.43 1.61 1.01 39 – – – –
He et al. 2023 2.40 1.75 – 20 – – – –

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

Visualization

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