OC 0366

0.35 UTI

0.41

C_N

0.34

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 41

Core radius and density 1.8 [pc], 1.7 [pc^-2]

C3 classification AA

C_N 0.41 Poorly populated
C_dens 0.34 Loose
C_C3 1.0 Very high 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 0366 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a close distance, below 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.

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0366 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–	89.651	-13.694	1.471	-1.707	1.715	25.664
Hao et al.	2022	89.632	-13.601	1.449	-1.742	1.713	–

💡 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–	–	1.8	–	3	0.250	–	–	–
Hao et al.	2022	–	1.80	–	3	0.250	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 18	12.2	89.47	-14.09	1.5	-2.01	1.64	26.55	0.11
CWWDL 14262	4.9	89.46	-14.1	1.49	-2.03	1.58	26.55	0.14

💡 Note: The % column shows the percentage of members that OC 0366 shares with each listed object.

Visualization

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