CWNU 2089

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0.60 UTI
0.5
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.4 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2089 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Near-solar metallicity 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 – 176.911 -62.792 0.208 -7.12 1.838 -3.279
Hunt & Reffert 2024 176.886 -62.79 0.222 -7.133 1.832 -4.175
Cavallo et al. 2024 176.9 -62.791 0.216 – – –
Hunt & Reffert 2023 176.886 -62.79 0.222 -7.133 1.832 -4.175
He et al. 2023 176.886 -62.788 0.233 -7.117 1.839 4.53

💡 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 – – – – – 2810* – –
Cavallo et al. 2024 3.91 4.16 – 282 0.040 – – –
Hunt & Reffert 2023 4.30 4.19 2.58 162 – – – –
He et al. 2023 4.17 4.70 – 224 – – – –

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

Visualization

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