OC 0624

0.01 UTI

0.37

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

N₅₀ (P>50% members) 37

Stellar density (N₅₀/rad) 6.4 [N/pc²]

C3 classification AB

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0624 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high 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, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

High extinction Metal-rich Very young

Data

🔍 Search references for OC 0624 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–	230.361	-60.884	1.174	-2.871	-4.057	-3.434
Hao et al.	2022	230.528	-60.841	1.152	-2.877	-4.048	–

💡 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–	–	3.17	–	5	0.611	–	–	–
Hao et al.	2022	–	3.17	–	5	0.611	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ASCC 79	97.3	229.73	-60.93	1.18	-3.05	-4.13	-7.27	0.91
CWWDL 14129	62.2	229.63	-60.98	1.19	-3.13	-4.11	-7.88	0.06
OC 0625	5.4	231.23	-61.06	1.17	-2.43	-4.22	-1.61	0.42

💡 Note: The % column shows the percentage of members that OC 0624 shares with each listed object.

Visualization

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