Ryu 24

0.20 UTI

0.0

C_N

0.86

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 21

Core radius and density 0.7 [pc], 4.3 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.86 Dense
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Ryu 24 is a sparse, dense object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Data

🔍 Search references for Ryu 24 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–	244.23	-51.53	0.368	-0.901	-2.237	-48.151
Bica et al.	2019	244.239	-51.537	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Visualization

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