LISC-III 3517

0.29 UTI

0.81

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.51

C_dup

C3 classification AA

Number of members (P>50%) 253

Radius (P>50% members) 25.0 [arcmin]

C_N 0.81 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.51 Likely unique

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

Overview

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LISC-III 3517 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 moderate extinction. It is catalogued as a near-solar metallicity cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Close Moderate extinction Near-solar metallicity

Data

🔍 Search references for LISC-III 3517 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	–	84.301	57.158	2.072	-3.159	-3.931	-6.325
Chi et al.	2023	83.406	57.349	2.008	-2.632	-3.336	–

💡 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	0.63	1.38	–	–	0.274	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 8	48.6	84.47	57.14	2.08	-3.22	-4.0	-6.46	0.87

💡 Note: The % column shows the percentage of members that LISC-III 3517 shares with each listed object.

Visualization

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