CWNU 2729

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0.46 UTI
0.31
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2729 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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 – 261.935 -38.371 0.637 -0.216 -1.923 -3.651
Hunt & Reffert 2024 261.915 -38.353 0.63 -0.208 -1.926 -3.648
Cavallo et al. 2024 261.956 -38.384 0.631 – – –
Hunt & Reffert 2023 261.915 -38.353 0.63 -0.208 -1.926 -3.648
He et al. 2023 261.945 -38.385 0.638 -0.227 -1.937 –

💡 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 – – – – – 465* – –
Cavallo et al. 2024 1.40 3.51 – 141 -0.260 – – –
Hunt & Reffert 2023 1.52 3.28 2.57 31 – – – –
He et al. 2023 1.45 3.20 – 398 – – – –

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

Visualization

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