LISC-III 3755

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0.15 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.26
Cdup
C3 classification AA
Number of members (P>50%) 155
Radius (P>50% members) 34.2 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.26 Possibly duplicate
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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LISC-III 3755 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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.

⚠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.

Very close Low extinction Near-solar metallicity

Data
🔍 Search references for LISC-III 3755 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 276.281 26.458 2.861 0.436 -5.383 -18.787
Chi et al. 2023 276.264 26.468 2.81 -0.147 -5.46 –

💡 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 0.40 0.50 – – 0.274 – 0.47 –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 179 73.5 276.5 26.43 2.88 0.53 -5.37 -19.11 0.83
CWWDL 14675 19.4 276.61 26.44 2.88 0.59 -5.34 -20.14 0.0

💡 Note: The % column shows the percentage of members that LISC-III 3755 shares with each listed object.

Visualization
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LISC-III 3755 UCC
Galactocentric position diagram