CWNU 2389

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0.60 UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.52 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 2389 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close Very high 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 – 253.473 -46.735 0.346 -1.177 -1.923 -44.383
Hunt & Reffert 2024 253.471 -46.736 0.367 -1.166 -1.959 -41.266
Cavallo et al. 2024 253.473 -46.735 0.36 – – –
Hunt & Reffert 2023 253.471 -46.736 0.367 -1.166 -1.959 -41.266
He et al. 2023 253.471 -46.744 0.365 -1.176 -1.924 -44.38

💡 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 – – – – – 871* – –
Cavallo et al. 2024 2.24 4.93 – 380 0.060 – – –
Hunt & Reffert 2023 2.54 5.22 2.62 97 – – – –
He et al. 2023 2.34 5.30 – 282 – – – –

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

Visualization

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