OC 0014

0.00 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.01

C_dup

C3 classification AB

Number of members (P>50%) 115

Radius (P>50% members) 2.2 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.01 Very likely duplicate

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

Overview

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OC 0014 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, old 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.

High extinction Metal-rich Old

Data

🔍 Search references for OC 0014 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	–	271.608	-21.402	0.462	-0.382	-1.506	21.661
Hao et al.	2022	271.617	-21.401	0.493	-0.371	-1.502	36.947

💡 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	–	4.85	–	1995	0.611	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0031	99.1	271.61	-21.4	0.45	-0.36	-1.51	20.64	0.75
Ryu 632	10.4	271.51	-21.36	0.33	-0.41	-1.56	83.45	0.14

💡 Note: The % column shows the percentage of members that OC 0014 shares with each listed object.

Visualization

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