CWNU 2292

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0.57 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2292 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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.
Distant 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 – 190.694 -61.915 0.293 -5.996 -0.671 -28.163
Hunt & Reffert 2024 190.701 -61.914 0.276 -5.998 -0.659 -29.811
Cavallo et al. 2024 190.691 -61.91 0.279 – – –
Hunt & Reffert 2023 190.701 -61.914 0.276 -5.998 -0.659 -29.811
He et al. 2023 190.68 -61.922 0.311 -5.988 -0.66 -27.05

💡 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 – – – – – 868* – –
Cavallo et al. 2024 3.12 4.21 – 380 0.310 – – –
Hunt & Reffert 2023 3.03 4.33 2.68 157 – – – –
He et al. 2023 2.57 3.85 – 891 – – – –

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

Visualization

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