LISC-III 3755

0.12 UTI

0.77

C_N

0.56

C_dens

1.0

C_C3

0.0

C_lit

0.26

C_dup

N_m (P>50%) 155

Core radius and density 2.0 [pc], 2.8 [pc^-2]

C3 classification AA

C_N 0.77 Rich
C_dens 0.56 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC-III 3755 is a rich, moderately 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.

⚠️ 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	99999–	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]	B_frac	BSS
UCC	99999–	0.4	0.54	–	–	0.119	–	0.47	–
Chi et al.	2023	0.40	0.54	–	–	0.119	–	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	0.71
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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