CWWDL 3284

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0.00 UTI
0.69
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 25.2 [N/pc2]
  • CN 0.69 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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CWWDL 3284 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 83.767 15.718 0.701 0.254 -2.386 10.424
Chi et al. 2023 83.766 15.716 0.69 0.238 -2.378 20.118

💡 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– – – – 33 -0.880 – – –
Chi et al. 2023 – – – 33 -0.880 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
COIN-Gaia 26 100.0 83.77 15.72 0.7 0.25 -2.4 10.42 0.81
LISC 0988 100.0 83.77 15.72 0.7 0.25 -2.39 10.42 0.04
UBC 75 98.9 83.77 15.72 0.7 0.26 -2.4 10.42 0.03

💡 Note: The % column shows the percentage of members that CWWDL 3284 shares with each listed object.

Visualization

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