OC 0422

0.00 UTI

0.36

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 8.0 [N/pc²]

C3 classification AA

C_N 0.36 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0422 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Near-solar metallicity Intermediate age

Data

🔍 Search references for OC 0422 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–	116.164	-28.385	0.246	-1.818	1.732	70.097
Hao et al.	2022	116.147	-28.369	0.259	-1.81	1.725	70.349

💡 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–	–	0.7	–	126	0.051	–	–	–
Hao et al.	2022	–	0.70	–	126	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Haffner 14	100.0	116.18	-28.38	0.25	-1.82	1.75	69.57	0.96
VVVX-Obasi 26	100.0	116.18	-28.38	0.25	-1.82	1.75	69.97	0.07

💡 Note: The % column shows the percentage of members that OC 0422 shares with each listed object.

Visualization

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