OCSN 35

0.02 UTI

0.34

C_N

0.46

C_dens

0.5

C_C3

0.0

C_lit

0.09

C_dup

N₅₀ (P>50% members) 34

Radius (P>50% members) 27.4 [arcmin]

C3 classification BB

C_N 0.34 Poorly populated
C_dens 0.46 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

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

Overview

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OCSN 35 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, below 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.

Close Low extinction Young

Data

🔍 Search references for OCSN 35 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–	347.008	45.288	2.066	-0.722	-3.541	-16.539
Qin et al.	2023	346.82	45.44	1.99	-0.66	-3.57	-14.21

💡 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–	0.6	0.46	–	50	–	–	–	–
Qin et al.	2023	0.60	0.46	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 824	91.2	346.9	45.45	2.04	-0.78	-3.31	-13.76	0.45
Theia 100	41.2	346.9	45.93	2.04	-0.81	-3.03	-12.98	0.1

💡 Note: The % column shows the percentage of members that OCSN 35 shares with each listed object.

Visualization

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