CWNU 508

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0.21 UTI
0.0
CN
0.2
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 15.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.2 Very loose
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 508 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Relatively close Moderate 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 – 338.561 62.624 0.981 -2.588 -2.536 -28.661
Hunt & Reffert 2024 338.587 62.602 0.959 -2.519 -2.451 -33.907
Cavallo et al. 2024 338.427 62.603 0.969 – – –
Hunt & Reffert 2023 338.587 62.602 0.959 -2.519 -2.451 -33.907
He et al. 2022 338.492 63.067 1.018 -2.816 -2.491 –
He et al. 2022 338.278 62.7 0.98 -2.63 -2.55 –

💡 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 – – – – – 139* – –
Cavallo et al. 2024 1.19 2.84 – 16 0.450 – – –
Hunt & Reffert 2023 1.00 3.05 2.05 32 – – – –
He et al. 2022 – 2.90 – 501 – – – –
He et al. 2022 0.87 3.00 – 32 0.169 – – –

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

Visualization

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