OCSN 106

0.00 UTI

0.0

C_N

0.18

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 21

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.5 Intermediate 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 106 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a 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 Young

Data

🔍 Search references for OCSN 106 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–	284.937	39.866	2.802	1.614	-1.646	-21.64
Qin et al.	2023	284.9	39.84	2.85	1.66	-1.58	-18.53

💡 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–	0.36	0.19	–	28	–	–	–	–
Qin et al.	2023	0.36	0.19	–	28	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 101	100.0	284.76	39.8	2.84	1.39	-1.74	-19.17	0.53
CWNU 510	12.0	287.67	39.52	2.84	1.83	-1.72	-19.98	0.22

💡 Note: The % column shows the percentage of members that OCSN 106 shares with each listed object.

Visualization

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