LISC 0901

0.52 UTI

0.83

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 309

Radius (P>50% members) 3.7 [arcmin]

C3 classification AB

C_N 0.83 Rich
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 0901 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~4.21 kpc) differs significantly from the median photometric distance (~3.02 kpc).

Note: This object shares a significant percentage of members with 3 later reported entries. See table with shared members information.

Distant Moderate extinction Very metal-poor Old

Data

🔍 Search references for LISC 0901 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–	133.923	-38.572	0.238	-4.983	3.86	53.527
Li et al.	2022	133.94	-38.573	0.24	-4.995	3.892	–

💡 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–	3.02	1.5	–	1000	-1.335	–	0.5	–
Li et al.	2022	3.02	1.50	–	1000	-1.335	–	0.50	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv
Theia 6978	52.4	133.92	-38.57	0.24	-5.01	3.85	51.67
UBC 1438	46.0	133.92	-38.57	0.23	-5.01	3.84	51.67
CWWDL 3104	26.5	133.93	-38.57	0.23	-5.01	3.84	49.16

💡 Note: The % column shows the percentage of members that LISC 0901 shares with each listed object.

Visualization

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