OC 0699

0.27 UTI

0.55

C_N

0.07

C_dens

0.75

C_C3

0.0

C_lit

0.98

C_dup

N_m (P>50%) 60

Core radius and density 4.9 [pc], 0.3 [pc^-2]

C3 classification AB

C_N 0.55 Moderately populated
C_dens 0.07 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.98 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0699 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Very high extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for OC 0699 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–	264.428	-32.065	0.186	-0.496	-1.873	-17.017
Hao et al.	2022	264.461	-32.046	0.145	-0.535	-1.906	-19.373

💡 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–	–	5.12	–	631	0.250	–	–	–
Hao et al.	2022	–	5.12	–	631	0.250	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
BDSB 167	1.7	264.39	-32.21	0.35	-0.88	-1.92	-22.69	0.11

💡 Note: The % column shows the percentage of members that OC 0699 shares with each listed object.

Visualization

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