CWNU 2631

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0.53 UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2631 is a poorly populated, very dense object of high 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, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Young

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 – 208.615 -63.076 0.31 -5.037 -2.007 –
Hunt & Reffert 2024 208.591 -63.08 0.301 -5.073 -2.03 -35.606
Cavallo et al. 2024 209.209 -63.019 0.301 – – –
Hunt & Reffert 2023 208.591 -63.08 0.301 -5.073 -2.03 -35.606
He et al. 2023 208.63 -63.077 0.328 -5.034 -2.003 -49.19

💡 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 – – – – – 451* – –
Cavallo et al. 2024 2.77 3.40 – 74 0.080 – – –
Hunt & Reffert 2023 3.02 3.08 2.78 36 – – – –
He et al. 2023 2.63 3.90 – 100 – – – –

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

Visualization

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