CWNU 2632

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0.31 UTI
0.32
CN
0.33
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2632 is a poorly populated, loose object of low 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)
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 – 189.405 -62.8 0.292 -5.333 -0.774 -7.792
Hunt & Reffert 2024 189.398 -62.791 0.284 -5.346 -0.79 -5.042
Cavallo et al. 2024 189.399 -62.801 0.284 – – –
Hunt & Reffert 2023 189.398 -62.791 0.284 -5.346 -0.79 -5.042
He et al. 2023 189.382 -62.812 0.315 -5.318 -0.785 -2.0

💡 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 – – – – – 343* – –
Cavallo et al. 2024 2.75 3.45 – 631 -0.350 – – –
Hunt & Reffert 2023 3.26 3.22 2.07 713 – – – –
He et al. 2023 2.82 3.50 – 708 – – – –

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

Visualization

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