CWNU 239

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0.00 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.3
Clit
0.0
Cdup
Stellar density (N50/rad) 15.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
CWNU 239 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 99999– 98.274 2.477 0.625 -2.322 -0.545 -24.694
Zhang et al. 2024 98.28 2.446 – – – –
Hunt & Reffert 2024 98.28 2.446 0.62 -2.321 -0.526 11.533
Cavallo et al. 2024 98.324 2.527 0.618 – – –
Hunt & Reffert 2023 98.28 2.446 0.62 -2.321 -0.526 11.533
He et al. 2022 98.268 2.457 0.62 -2.34 -0.54 –

💡 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] Bfrac BSS
UCC 99999– 1.5 2.56 2.79 13 0.080 1473 – –
Zhang et al. 2024 – – – – -0.069(1) – – –
Hunt & Reffert 2024 – – – – – 1473(1) – –
Cavallo et al. 2024 1.62 2.56 – 11 0.080 – – –
Hunt & Reffert 2023 1.50 2.44 2.79 13 – – – –
He et al. 2022 1.45 2.82 – 25 0.457 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 3775 100.0 98.27 2.46 0.63 -2.32 -0.53 -24.69 0.0
LISC-III 1682 100.0 98.27 2.47 0.63 -2.29 -0.53 -17.72 0.15
UBC 1330 100.0 98.28 2.46 0.62 -2.33 -0.56 -17.72 0.49

💡 Note: The % column shows the percentage of members that CWNU 239 shares with each listed object.

Visualization

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