CWNU 3069

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0.08 UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.0
Clit
0.44
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.44 Possibly duplicate

Overview

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CWNU 3069 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Low extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 116.94 -24.704 0.207 -1.543 1.785 –
He et al. 2023 116.952 -24.704 0.219 -1.528 1.785 –

💡 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
He et al. 2023 4.17 1.00 – 501 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWL 2073 56.0 116.95 -24.7 0.21 -1.53 1.84 70.75 0.22
CWWL 1438 32.0 116.9 -24.76 0.23 -1.57 1.86 62.24 0.06

💡 Note: The % column shows the percentage of members that CWNU 3069 shares with each listed object.

Visualization

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