LISC 1351

0.52 UTI

0.6

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 70

Radius (P>50% members) 2.0 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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LISC 1351 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.13 kpc) differs significantly from the median photometric distance (~1.91 kpc).

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 1351 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	–	308.924	36.572	0.319	-2.113	-4.979	-14.861
Li et al.	2022	308.948	36.608	0.321	-2.186	-4.866	–

💡 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	1.91	3.30	–	100	0.274	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1102	88.6	308.92	36.57	0.32	-2.1	-5.0	-23.18	0.13
CWNU 118	44.3	308.93	36.57	0.32	-2.1	-5.01	–	0.0

💡 Note: The % column shows the percentage of members that LISC 1351 shares with each listed object.

Visualization

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