Slizhevsky 250

0.11 UTI

0.0

C_N

0.06

C_dens

0.5

C_C3

0.0

C_lit

0.96

C_dup

N₅₀ (P>50% members) 14

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Slizhevsky 250 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for Slizhevsky 250 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–	199.429	-63.44	0.19	-6.734	-1.005	-25.02
Dias et al.	2026	199.345	-63.466	0.195	-6.73	-1.006	–

💡 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–	4.78	2.65	–	6	0.131	–	–	–
Dias et al.	2026	4.78	2.65	–	6	0.131	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1643	4.0	199.04	-63.42	0.2	-6.84	-0.97	-25.56	0.43

💡 Note: The % column shows the percentage of members that Slizhevsky 250 shares with each listed object.

Visualization

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