CWNU 2637

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0.39 UTI
0.47
CN
0.22
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.0 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2637 is a poorly populated, very loose 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, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Near-solar metallicity Very 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 – 90.052 21.486 0.27 -0.193 -1.429 –
Hunt & Reffert 2024 90.073 21.486 0.279 -0.217 -1.418 –
Cavallo et al. 2024 90.049 21.537 0.279 – – –
Hunt & Reffert 2023 90.073 21.486 0.279 -0.217 -1.418 –
He et al. 2023 89.96 21.395 0.286 -0.2 -1.445 –

💡 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 – – – – – 852* – –
Cavallo et al. 2024 3.47 3.05 – 41 0.470 – – –
Hunt & Reffert 2023 3.17 3.21 2.47 15 – – – –
He et al. 2023 3.63 3.45 – 9 – – – –

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

Visualization

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