OC 0262

0.30 UTI

0.46

C_N

0.3

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 46

Core radius and density 2.4 [pc], 1.5 [pc^-2]

C3 classification AB

C_N 0.46 Poorly populated
C_dens 0.3 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0262 is a poorly populated, 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.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0262 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–	50.177	58.928	0.909	0.478	-1.664	-17.567
Hao et al.	2022	50.127	58.946	0.911	0.459	-1.642	68.822

💡 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–	–	1.75	–	5	0.250	–	–	–
Hao et al.	2022	–	1.75	–	5	0.250	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1131	100.0	50.2	58.95	0.92	0.55	-1.61	-17.27	0.28
Theia 1713	100.0	50.22	58.93	0.92	0.51	-1.61	-17.57	0.02

💡 Note: The % column shows the percentage of members that OC 0262 shares with each listed object.

Visualization

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