OCSN 214

0.00 UTI

0.67

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 84

Stellar density (N₅₀/rad) 163.0 [N/pc²]

C3 classification AA

C_N 0.67 Moderately populated
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

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OCSN 214 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported 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.

Very close Low extinction Very young

Data

🔍 Search references for OCSN 214 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–	242.203	-39.072	6.282	-9.868	-23.507	-2.454
Qin et al.	2023	242.13	-39.09	6.27	-9.87	-23.49	-1.26

💡 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–	0.19	0.59	–	4	–	–	–	–
Qin et al.	2023	0.19	0.59	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1014	100.0	242.2	-39.07	6.28	-9.91	-23.43	-2.54	0.31
OC 0666	51.2	242.17	-39.06	6.31	-10.0	-23.48	-2.45	0.49
CWNU 1004	20.2	240.21	-41.68	6.24	-10.93	-23.51	-2.11	0.41

💡 Note: The % column shows the percentage of members that OCSN 214 shares with each listed object.

Visualization

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