LISC 0275

0.08 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

C3 classification AA

Number of members (P>50%) 100

Radius (P>50% members) 2.6 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

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LISC 0275 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an extremely metal-poor, 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.

(*): The parallax distance estimate (~3.36 kpc) differs significantly from the median photometric distance (~1.74 kpc).

Relatively close Moderate extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 0275 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	–	359.585	61.189	0.298	-3.218	-1.699	-69.755
Li et al.	2022	359.25	61.102	0.309	-3.125	-1.632	–

💡 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	1.74	1.88	–	100	-2.721	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Collinder 461	85.0	359.61	61.21	0.29	-3.25	-1.72	-69.41	0.96
OC 0213	45.0	359.61	61.21	0.29	-3.24	-1.71	-58.93	0.0

💡 Note: The % column shows the percentage of members that LISC 0275 shares with each listed object.

Visualization

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