CWNU 1083

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0.66 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 11.5 [N/pc2]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1083 is a rich, very dense object of very 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, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 90 along with CWNU_1096, and of multiple system 30 along with Theia_31 and CWNU_1096.

Palma et al. (2025)
Classified as optical pair P609, along with OC_0450.

Cavallo et al. (2024)
Silver 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– 125.88 -41.172 2.938 -7.122 10.114 15.357
Liu et al. 2025 126.14 -41.02 2.93 -7.14 10.11 30.68
Cavallo et al. 2024 126.075 -40.891 2.928 – – –
Hunt & Reffert 2023 126.135 -41.018 2.93 -7.138 10.109 30.681
He et al. 2022 125.667 -41.525 2.927 -7.1 10.014 –

💡 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– 0.37 0.335 1.19 10 -0.150 – – –
Liu et al. 2025 0.37 0.10 – 11 – – – –
Cavallo et al. 2024 0.37 1.24 – 13 -0.150 – – –
Hunt & Reffert 2023 0.34 0.57 1.19 8 – – – –
He et al. 2022 – 0.05 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 201 81.1 125.99 -41.07 2.94 -7.12 10.13 14.81 0.01
CWWDL 14610 36.1 126.15 -40.96 2.94 -7.12 10.14 15.09 0.0

💡 Note: The % column shows the percentage of members that CWNU 1083 shares with each listed object.

Visualization

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