OC 0182

0.00 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 79

Radius (P>50% members) 2.3 [arcmin]

C_N 0.64 Moderately 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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OC 0182 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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 moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

High extinction Near-solar metallicity Young

Data

🔍 Search references for OC 0182 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	–	337.073	59.131	0.263	-3.341	-2.387	87.836
Hao et al.	2022	337.052	59.12	0.277	-3.339	-2.383	–

💡 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	–	3.82	–	50	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Berkeley 95	100.0	337.07	59.13	0.26	-3.34	-2.37	34.0	0.97
OC 0183	44.3	337.08	59.14	0.28	-3.33	-2.38	87.84	0.0
CWWDL 2544	34.2	337.06	59.1	0.26	-3.29	-2.38	87.84	0.05

💡 Note: The % column shows the percentage of members that OC 0182 shares with each listed object.

Visualization

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