OC 0418

0.01 UTI

0.37

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.03

C_dup

C3 classification BB

Number of members (P>50%) 37

Radius (P>50% members) 3.0 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 0418 is a poorly populated, very dense object of intermediate 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, 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.

Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0418 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	–	113.659	-28.079	0.329	-2.825	3.704	–
Hao et al.	2022	113.67	-28.069	0.327	-2.813	3.728	–

💡 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	–	1.78	–	8	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 464	97.3	113.58	-28.12	0.32	-2.83	3.68	93.7	0.23
CWWDL 144	89.2	113.66	-28.08	0.33	-2.81	3.7	–	0.0

💡 Note: The % column shows the percentage of members that OC 0418 shares with each listed object.

Visualization

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