CWNU 2629

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0.56 UTI
0.64
CN
0.91
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 0.91 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2629 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 massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 216.47 -59.032 0.331 -5.67 -2.65 -43.774
Hunt & Reffert 2024 216.531 -59.049 0.325 -5.658 -2.673 -47.619
Cavallo et al. 2024 216.45 -59.039 0.324 – – –
Hunt & Reffert 2023 216.531 -59.049 0.325 -5.658 -2.673 -47.619
He et al. 2023 216.53 -59.04 0.359 -5.645 -2.649 -10.05

💡 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 – – – – – 1395* – –
Cavallo et al. 2024 3.55 4.42 – 68 0.100 – – –
Hunt & Reffert 2023 2.69 4.21 2.89 244 – – – –
He et al. 2023 2.40 4.70 – 141 – – – –

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

Visualization

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