CWNU 1004

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0.41 UTI
0.41
CN
0.64
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.2 [N/pc2]
  • CN 0.41 Poorly populated
  • Cdens 0.64 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1004 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 240.206 -41.679 6.245 -10.929 -23.513 -2.11
Cavallo et al. 2024 239.844 -42.107 6.257 – – –
Hunt & Reffert 2023 239.73 -42.008 6.257 -11.058 -23.509 -2.013
He et al. 2022 239.698 -42.032 6.259 -11.103 -23.516 –

💡 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– 0.16 1.98 1.22 11 0.290 – – –
Cavallo et al. 2024 0.16 1.98 – 129 0.290 – – –
Hunt & Reffert 2023 0.16 1.17 1.22 6 – – – –
He et al. 2022 – 2.95 – 11 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1014 43.9 242.2 -39.07 6.28 -9.91 -23.43 -2.54 0.31
OCSN 214 41.5 242.2 -39.07 6.28 -9.87 -23.51 -2.45 0.0

💡 Note: The % column shows the percentage of members that CWNU 1004 shares with each listed object.

Visualization

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