OC 0696

0.03 UTI

0.0

C_N

0.32

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

N_m (P>50%) 23

Core radius and density 1.1 [pc], 1.6 [pc^-2]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.32 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0696 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 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 0696 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–	260.873	-32.051	0.594	-1.212	-2.466	-56.808
Hao et al.	2022	260.852	-32.057	0.593	-1.22	-2.467	–

💡 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–	–	2.43	–	10	0.022	–	–	–
Hao et al.	2022	–	2.43	–	10	0.022	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UFMG 66	84.0	260.88	-32.05	0.59	-1.2	-2.46	-56.81	0.2

💡 Note: The % column shows the percentage of members that OC 0696 shares with each listed object.

Visualization

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