OCSN 29

0.02 UTI

0.72

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.04

C_dup

N₅₀ (P>50% members) 93

Stellar density (N₅₀/rad) 10.9 [N/pc²]

C3 classification AA

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OCSN 29 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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.

Close Low extinction Very young

Data

🔍 Search references for OCSN 29 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–	339.149	37.722	2.035	-1.721	-6.187	-13.077
Qin et al.	2023	339.08	37.79	2.05	-1.81	-6.15	-13.7

💡 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–	0.57	0.4	–	16	–	–	–	–
Qin et al.	2023	0.57	0.40	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 39	95.7	339.22	37.76	2.04	-1.76	-6.04	-13.08	0.83
CWWDL 14543	34.4	339.72	37.29	2.01	-1.55	-6.12	-13.97	0.12
FoF 2379	14.0	339.63	38.15	1.98	-1.56	-5.8	-21.27	0.16

💡 Note: The % column shows the percentage of members that OCSN 29 shares with each listed object.

Visualization

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