CWWDL 10843

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0.03 UTI
0.38
CN
0.85
Cdens
0.38
CC3
0.0
Clit
0.1
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.85 Dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.1 Likely duplicate

Overview

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CWWDL 10843 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Near-solar metallicity Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 93.929 22.623 0.517 -0.355 -1.661 –
Chi et al. 2023 93.911 22.613 0.51 -0.389 -1.602 -6.772

💡 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
Chi et al. 2023 – – – 1 0.440 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1305 89.5 93.94 22.62 0.52 -0.35 -1.67 – 0.38
Teutsch 170 15.8 93.85 22.85 0.45 -0.31 -1.61 – 0.07

💡 Note: The % column shows the percentage of members that CWWDL 10843 shares with each listed object.

Visualization

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