CWNU 1083

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0.56 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 39.9 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely 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 (see Parameters). It is rarely studied in the literature.

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

Very close Low extinction Near-solar metallicity Very young

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 – 125.88 -41.172 2.938 -7.122 10.114 15.357
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] Bfr BSS
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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