LISC-III 3249

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0.05 UTI
0.35
CN
0.34
Cdens
0.38
CC3
0.0
Clit
0.26
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.26 Possibly duplicate

Overview

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LISC-III 3249 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a very close* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity 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.

(*): The parallax distance estimate (~0.49 kpc) differs significantly from the median photometric distance (~0.72 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 260.883 -62.085 2.055 -0.564 -8.736 9.264
Chi et al. 2023 261.189 -61.325 1.995 -0.713 -8.323 –

💡 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– 0.72 0.5 – – 0.274 – 0.45 –
Chi et al. 2023 0.72 0.50 – – 0.274 – 0.45 –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi 24 74.3 260.78 -62.72 2.06 -0.45 -8.98 9.22 0.97
OC 0639 5.7 261.07 -62.46 2.04 -0.42 -8.97 8.85 0.0

💡 Note: The % column shows the percentage of members that LISC-III 3249 shares with each listed object.

Visualization

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