LISC 3404

0.12 UTI

0.72

C_N

0.7

C_dens

0.75

C_C3

0.0

C_lit

0.27

C_dup

C3 classification AB

Number of members (P>50%) 93

Radius (P>50% members) 16.0 [arcmin]

C_N 0.72 Moderately populated
C_dens 0.7 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC 3404 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 3404 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	–	288.857	-4.203	0.905	-0.546	-4.959	-1.488
Li et al.	2022	288.875	-4.187	0.903	-0.565	-4.993	–

💡 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
Li et al.	2022	0.91	1.65	–	200	-0.419	–	0.52	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 356	73.1	288.86	-4.2	0.91	-0.56	-4.94	-1.55	0.65
CWWDL 14312	59.1	288.89	-4.2	0.91	-0.55	-4.96	-8.13	0.0

💡 Note: The % column shows the percentage of members that LISC 3404 shares with each listed object.

Visualization

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