LISC 3279

0.07 UTI

0.64

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.15

C_dup

C3 classification AB

Number of members (P>50%) 78

Radius (P>50% members) 3.9 [arcmin]

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

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LISC 3279 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~1.59 kpc) differs significantly from the median photometric distance (~1.12 kpc).

Relatively close Moderate extinction Very metal-poor Intermediate age

Data

🔍 Search references for LISC 3279 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	–	289.995	15.153	0.63	-1.692	-5.286	3.243
Li et al.	2022	290.0	15.146	0.63	-1.669	-5.225	–

💡 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	1.12	2.00	–	300	-1.335	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 9918	88.5	290.0	15.15	0.63	-1.69	-5.28	-4.26	0.05
UBC 361	84.6	290.0	15.15	0.63	-1.7	-5.29	-4.26	0.69

💡 Note: The % column shows the percentage of members that LISC 3279 shares with each listed object.

Visualization

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