LISC-III 3449

0.02 UTI

0.78

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.04

C_dup

C3 classification AA

Number of members (P>50%) 173

Radius (P>50% members) 22.2 [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 0.04 Very likely duplicate

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

Overview

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LISC-III 3449 is a rich, very dense object of very 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 metal-poor cluster (see Parameters). It was recently reported 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.

Very close Low extinction Metal-poor

Data

🔍 Search references for LISC-III 3449 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	–	279.688	5.559	2.096	1.103	-4.878	-25.005
Chi et al.	2023	280.063	6.373	2.034	0.835	-4.849	–

💡 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
Chi et al.	2023	0.44	0.45	–	–	-0.642	–	0.49	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 210	96.5	279.66	5.45	2.11	1.26	-4.95	-24.82	1.0
OC 0066	9.8	279.46	5.25	2.13	1.22	-4.99	-25.29	0.0

💡 Note: The % column shows the percentage of members that LISC-III 3449 shares with each listed object.

Visualization

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