OC 0524

0.01 UTI

0.0

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.04

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 35.1 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0524 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Low extinction Metal-rich Very young

Data

🔍 Search references for OC 0524 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–	147.809	-53.178	0.387	-5.795	3.622	-23.637
Hao et al.	2022	147.804	-53.178	0.386	-5.805	3.587	–

💡 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–	–	0.53	–	4	0.611	–	–	–
Hao et al.	2022	–	0.53	–	4	0.611	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Pismis 16	96.0	147.81	-53.18	0.37	-5.75	3.52	-19.01	0.88

💡 Note: The % column shows the percentage of members that OC 0524 shares with each listed object.

Visualization

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