CWNU 2160

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0.35 UTI
0.0
CN
0.48
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.48 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2160 is a sparse, loose object of high C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Very distant High extinction Very metal-poor Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.111 48.916 0.16 -2.538 -3.805 -62.876
Hunt & Reffert 2024 307.111 48.907 0.145 -2.527 -3.805 -62.857
Cavallo et al. 2024 307.115 48.916 0.138 – – –
Hunt & Reffert 2023 307.111 48.907 0.145 -2.527 -3.805 -62.857
He et al. 2023 307.117 48.901 0.14 -2.549 -3.823 -62.01

💡 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 – – – – – 498* – –
Cavallo et al. 2024 3.28 3.64 – 603 -1.340 – – –
Hunt & Reffert 2023 7.61 3.09 1.76 199 – – – –
He et al. 2023 5.37 2.35 – 708 – – – –

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

Visualization

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