LISC 3392

0.56 UTI

0.78

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 178

Radius (P>50% members) 21.9 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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LISC 3392 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close^* distance, below the mid-plane, affected by low extinction. It is catalogued as an extremely metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~0.82 kpc) differs significantly from the median photometric distance (~0.47 kpc).

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Very close Low extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 3392 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	–	104.352	-21.339	1.215	-3.463	3.253	36.609
Li et al.	2022	104.419	-21.397	1.21	-3.435	3.272	–

💡 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	0.47	0.33	–	100	-5.024	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 91	97.2	104.32	-21.31	1.22	-3.45	3.25	36.54	0.1
OC 0395	58.4	104.35	-21.28	1.21	-3.49	3.26	36.28	0.0
CWWDL 14305	25.3	104.37	-21.34	1.22	-3.51	3.28	34.91	0.0

💡 Note: The % column shows the percentage of members that LISC 3392 shares with each listed object.

Visualization

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