OC 0232

0.31 UTI

0.0

C_N

0.28

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 24

Radius (P>50% members) 5.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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OC 0232 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for OC 0232 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	–	17.628	62.743	0.372	-2.061	-0.343	–
Hunt & Reffert	2024	17.573	62.732	0.364	-2.065	-0.352	–
Cavallo et al.	2024	17.636	62.749	0.363	–	–	–
Hunt & Reffert	2023	17.573	62.732	0.364	-2.065	-0.352	–
Hao et al.	2022	17.852	62.729	0.366	-2.019	-0.379	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	415*	–	–
Cavallo et al.	2024	2.68	2.57	–	107	0.320	–	–	–
Hunt & Reffert	2023	2.51	2.53	1.12	76	–	–	–	–
Hao et al.	2022	–	4.15	–	13	0.611	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 8488	56.0	17.49	62.79	0.35	-2.06	-0.33	-82.23	0.05

💡 Note: The % column shows the percentage of members that OC 0232 shares with each listed object.

Visualization

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