OC 0032

0.00 UTI

0.35

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification DA

Number of members (P>50%) 35

Radius (P>50% members) 3.5 [arcmin]

C_N 0.35 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 0032 is a poorly populated, very dense object of intermediate 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, 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 0032 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	–	277.259	-12.725	0.48	0.623	-1.657	88.268
Hao et al.	2022	277.255	-12.714	0.524	0.639	-1.638	–

💡 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	–	2.98	–	10	0.112	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1020	100.0	277.26	-12.72	0.46	0.62	-1.65	10.83	0.66
CWNU 506	94.3	277.25	-12.72	0.48	0.64	-1.67	17.92	0.0
CWNU 44	88.6	277.26	-12.72	0.47	0.61	-1.66	18.06	0.0
HSC 210	14.3	277.31	-12.7	0.57	0.55	-1.62	–	0.06

💡 Note: The % column shows the percentage of members that OC 0032 shares with each listed object.

Visualization

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