LISC 3170

0.07 UTI

0.44

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification AB

Number of members (P>50%) 44

Radius (P>50% members) 3.4 [arcmin]

C_N 0.44 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

ℹ️

LISC 3170 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 3170 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	214.653	-62.658	0.461	-3.909	-2.547	–
Li et al.	2022	214.64	-62.654	0.459	-3.984	-2.627	–

💡 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	2.19	2.03	–	100	0.274	–	0.36	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2819	93.2	214.66	-62.66	0.46	-3.9	-2.53	-5.0	0.06
UFMG 60	84.1	214.67	-62.66	0.46	-3.88	-2.53	-5.0	0.5

💡 Note: The % column shows the percentage of members that LISC 3170 shares with each listed object.

Visualization

ℹ️