OC 0534

0.02 UTI

0.7

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AA

Number of members (P>50%) 89

Radius (P>50% members) 2.8 [arcmin]

C_N 0.7 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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OC 0534 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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.

Moderate extinction Near-solar metallicity Old

Data

🔍 Search references for OC 0534 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	–	149.032	-60.183	0.333	-5.875	5.223	0.809
Hao et al.	2022	149.033	-60.182	0.341	-5.867	5.252	-1.055

💡 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
Hao et al.	2022	–	2.35	–	1585	0.112	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 676	96.6	149.03	-60.18	0.33	-5.88	5.22	-0.08	0.54
Theia 6242	96.6	149.03	-60.18	0.33	-5.87	5.22	0.66	0.04
CWWDL 214	46.1	149.03	-60.18	0.33	-5.89	5.21	1.81	0.0

💡 Note: The % column shows the percentage of members that OC 0534 shares with each listed object.

Visualization

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