LISC 1274

0.46 UTI

0.55

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 60

Radius (P>50% members) 2.4 [arcmin]

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 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 1274 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.54 kpc) differs significantly from the median photometric distance (~1.45 kpc).

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

Relatively close Low extinction Near-solar metallicity Old

Data

🔍 Search references for LISC 1274 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	–	180.96	-63.61	0.282	-5.106	0.914	–
Li et al.	2022	180.949	-63.62	0.279	-5.223	0.905	–

💡 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	1.45	0.88	–	2400	-0.419	–	0.53	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1512	88.3	180.96	-63.61	0.28	-5.09	0.93	–	0.23

💡 Note: The % column shows the percentage of members that LISC 1274 shares with each listed object.

Visualization

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