OC 0116

0.10 UTI

0.42

C_N

0.43

C_dens

0.75

C_C3

0.0

C_lit

0.31

C_dup

N_m (P>50%) 42

Core radius and density 1.1 [pc], 2.2 [pc^-2]

C3 classification AB

C_N 0.42 Poorly populated
C_dens 0.43 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0116 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 possibly a duplicate object, which shares a significant 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 0116 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–	304.688	40.044	0.569	-3.407	-5.19	-47.159
Hao et al.	2022	304.685	40.047	0.559	-3.359	-5.184	–

💡 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–	–	2.66	–	8	0.265	–	–	–
Hao et al.	2022	–	2.66	–	8	0.265	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 11640	95.2	304.68	40.05	0.57	-3.42	-5.19	-41.86	0.12
UBC 375	69.0	304.64	40.05	0.57	-3.46	-5.21	46.38	0.41

💡 Note: The % column shows the percentage of members that OC 0116 shares with each listed object.

Visualization

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