CWNU 2601

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0.57 UTI
0.35
CN
0.85
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.85 Dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2601 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Very distant Moderate extinction 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 – 159.209 -61.567 0.162 -5.126 2.142 13.578
Hu & Soubiran 2025 159.21 -61.566 – – – –
Hunt & Reffert 2024 159.207 -61.573 0.172 -5.135 2.145 13.619
Cavallo et al. 2024 159.21 -61.566 0.172 – – –
Hunt & Reffert 2023 159.207 -61.573 0.172 -5.135 2.145 13.619
He et al. 2023 159.203 -61.568 0.178 -5.129 2.142 13.58

💡 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 – – – – – 389* – –
Cavallo et al. 2024 5.01 0.92 – 589 0.600 – – –
Hunt & Reffert 2023 5.33 1.73 0.95 156 – – – –
He et al. 2023 4.90 1.65 – 398 – – – –

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

Visualization

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