CWNU 2529

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0.60 UTI
0.51
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2529 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Very distant High extinction Very massive Near-solar metallicity Young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 169.756 -61.456 0.121 -5.376 1.791 -46.68
Hunt & Reffert 2024 169.764 -61.458 0.117 -5.391 1.798 36.973
Cavallo et al. 2024 169.683 -61.461 0.112 – – –
Hunt & Reffert 2023 169.764 -61.458 0.117 -5.391 1.798 36.973
He et al. 2023 169.767 -61.457 0.125 -5.369 1.773 –

💡 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 – – – – – 5701* – –
Cavallo et al. 2024 4.29 4.23 – 76 -0.010 – – –
Hunt & Reffert 2023 8.47 4.74 2.90 29 – – – –
He et al. 2023 9.77 6.90 – 4 – – – –

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

Visualization

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