CWNU 2792

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0.51 UTI
0.34
CN
0.98
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.98 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2792 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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)
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 – 225.08 -58.379 0.408 -4.474 -2.806 -26.829
Hunt & Reffert 2024 225.091 -58.36 0.412 -4.468 -2.794 -38.806
Cavallo et al. 2024 225.058 -58.368 0.409 – – –
Hunt & Reffert 2023 225.091 -58.36 0.412 -4.468 -2.794 -38.806
He et al. 2023 225.039 -58.411 0.405 -4.516 -2.812 -26.4

💡 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 – – – – – 651* – –
Cavallo et al. 2024 1.97 4.02 – 219 0.240 – – –
Hunt & Reffert 2023 2.26 4.29 2.41 100 – – – –
He et al. 2023 2.24 4.50 – 224 – – – –

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

Visualization

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