CWNU 1529

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0.46 UTI
0.38
CN
0.65
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1529 is a poorly populated, moderately dense object of high 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, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 247.786 -50.225 0.604 -1.812 -4.728 -32.194
Hunt & Reffert 2024 247.862 -50.23 0.584 -1.794 -4.693 -18.242
Cavallo et al. 2024 247.735 -50.26 0.59 – – –
Hunt & Reffert 2023 247.862 -50.23 0.584 -1.794 -4.693 -18.242
He et al. 2023 247.767 -50.232 0.608 -1.812 -4.739 -35.03

💡 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 – – – – – 742* – –
Cavallo et al. 2024 1.56 4.25 – 23 0.190 – – –
Hunt & Reffert 2023 1.57 4.12 2.89 29 – – – –
He et al. 2023 1.58 4.65 – 10 – – – –

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

Visualization

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