CWNU 2288

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0.45 UTI
0.52
CN
0.72
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.72 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2288 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction 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 – 271.745 -18.242 0.512 0.438 -0.448 –
Hunt & Reffert 2024 271.729 -18.252 0.506 0.436 -0.468 –
Cavallo et al. 2024 271.734 -18.244 0.503 – – –
Hunt & Reffert 2023 271.729 -18.252 0.506 0.436 -0.468 –
He et al. 2023 271.749 -18.249 0.531 0.401 -0.456 –

💡 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 – – – – – 329* – –
Cavallo et al. 2024 1.68 3.56 – 209 0.050 – – –
Hunt & Reffert 2023 1.88 3.76 2.38 63 – – – –
He et al. 2023 1.74 4.20 – 112 – – – –

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

Visualization

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