LISC-III 3785

0.15 UTI

0.25

C_N

0.17

C_dens

0.75

C_C3

0.0

C_lit

0.64

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification BA

C_N 0.25 Poorly populated
C_dens 0.17 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC-III 3785 is a poorly populated, very loose object of 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 very metal-poor cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Very metal-poor

Data

🔍 Search references for LISC-III 3785 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–	270.594	22.702	3.467	-1.316	-7.273	-18.737
Chi et al.	2023	270.709	22.617	3.553	-1.4	-7.091	–

💡 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–	0.26	0.75	–	–	-1.335	–	0.47	–
Chi et al.	2023	0.26	0.75	–	–	-1.335	–	0.47	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 11	36.0	270.09	21.47	3.39	-1.34	-7.63	-18.06	0.19

💡 Note: The % column shows the percentage of members that LISC-III 3785 shares with each listed object.

Visualization

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