OC 0314

0.20 UTI

0.38

C_N

0.12

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 38

Core radius and density 2.3 [pc], 0.6 [pc^-2]

C3 classification BB

C_N 0.38 Poorly populated
C_dens 0.12 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0314 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

High extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0314 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–	90.997	20.284	0.514	1.134	-2.548	96.226
Hao et al.	2022	90.991	20.277	0.535	1.123	-2.57	37.59

💡 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–	–	3.09	–	10	0.250	–	–	–
Hao et al.	2022	–	3.09	–	10	0.250	–	–	–

Visualization

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