LISC 3355

0.00 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 110

Radius (P>50% members) 7.9 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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LISC 3355 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close^* distance, above 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 very 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 (~1.38 kpc) differs significantly from the median photometric distance (~0.78 kpc).

Close Moderate extinction Very metal-poor Intermediate age

Data

🔍 Search references for LISC 3355 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	–	249.706	-44.762	0.725	-0.801	-2.726	-18.075
Li et al.	2022	249.7	-44.785	0.715	-0.797	-2.729	–

💡 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	0.78	1.33	–	900	-1.335	–	0.39	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 319	100.0	249.72	-44.76	0.72	-0.79	-2.73	-18.07	0.74
CWWDL 13986	72.7	249.68	-44.75	0.72	-0.79	-2.73	-22.37	0.0

💡 Note: The % column shows the percentage of members that LISC 3355 shares with each listed object.

Visualization

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