OC 0341

0.00 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 137

Stellar density (N₅₀/rad) 78.7 [N/pc²]

C3 classification AA

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

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

OC 0341 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very 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.

⚠️ 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 0341 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	86.661	0.112	2.403	-0.382	-0.69	-0.055
Hao et al.	2022	86.667	0.149	2.387	-0.464	-0.737	8.668

💡 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–	–	1.66	–	1	0.051	–	–	–
Hao et al.	2022	–	1.66	–	1	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 2068	100.0	86.64	0.11	2.41	-0.51	-0.76	8.42	0.66
OCSN 62	99.3	86.66	0.11	2.41	-0.37	-0.72	8.03	0.0
FoF 2382	17.5	86.68	0.18	2.41	-0.92	-0.87	-10.2	0.0
NGC 2071	16.8	86.78	0.31	2.29	-1.0	-1.0	–	0.46

💡 Note: The % column shows the percentage of members that OC 0341 shares with each listed object.

Visualization

ℹ️