CWNU 1013

(OCSN 163)

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0.43 UTI
0.52
CN
0.38
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 77.7 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.38 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1013 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly studied in the literature.

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

Cavallo et al. (2024)
Gold 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– 104.811 -34.472 4.302 -11.807 8.072 14.647
Cavallo et al. 2024 104.735 -34.441 4.298 – – –
Hunt & Reffert 2023 104.552 -33.058 4.289 -11.985 8.057 13.672
Qin et al. 2023 104.96 -35.32 4.4 -12.14 8.29 14.63
He et al. 2022 104.716 -35.031 4.37 -11.978 8.328 –

💡 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– 0.23 0.34 0.47 36 0.190 – – –
Cavallo et al. 2024 0.23 0.49 – 37 0.190 – – –
Hunt & Reffert 2023 0.23 0.57 0.47 402 – – – –
Qin et al. 2023 0.25 0.19 – 35 – – – –
He et al. 2022 – 0.05 – 32 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1162 3.8 106.28 -34.46 3.88 -11.45 7.15 16.86 0.22

💡 Note: The % column shows the percentage of members that CWNU 1013 shares with each listed object.

Visualization

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