OC 0362

0.47 UTI

0.62

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 74

Radius (P>50% members) 11.4 [arcmin]

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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OC 0362 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low 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 moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Low extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0362 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	–	90.894	-9.787	1.193	-2.107	1.642	39.523
Hao et al.	2022	90.953	-9.799	1.195	-2.127	1.549	30.279

💡 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]	Bfr	BSS
Hao et al.	2022	–	0.22	–	5	0.274	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14261	39.2	90.89	-9.75	1.16	-2.05	1.62	44.56	0.01
OC 0361	33.8	90.56	-9.92	1.23	-2.02	1.77	18.13	0.35
Theia 15	32.4	90.87	-9.75	1.18	-2.24	1.62	46.29	0.02

💡 Note: The % column shows the percentage of members that OC 0362 shares with each listed object.

Visualization

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