LISC-III 3645

0.00 UTI

0.33

C_N

0.78

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 3.9 [N/pc²]

C3 classification BA

C_N 0.33 Poorly populated
C_dens 0.78 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC-III 3645 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity 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 Near-solar metallicity

Data

🔍 Search references for LISC-III 3645 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	99999–	79.513	18.092	2.723	0.097	-5.643	24.351
Chi et al.	2023	79.722	17.899	2.696	0.039	-5.714	–

💡 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]	B_frac	BSS
UCC	99999–	0.46	0.8	–	–	0.274	–	0.44	–
Chi et al.	2023	0.46	0.80	–	–	0.274	–	0.44	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 111	100.0	79.29	18.61	2.83	-0.11	-5.87	21.26	0.46
CWNU 1007	57.6	79.33	18.53	2.79	0.04	-5.75	19.17	0.41

💡 Note: The % column shows the percentage of members that LISC-III 3645 shares with each listed object.

Visualization

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