OC 0379

0.00 UTI

0.29

C_N

0.78

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BC

Number of members (P>50%) 29

Radius (P>50% members) 7.9 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.78 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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OC 0379 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 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.

Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0379 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	–	107.565	-12.446	0.841	-3.047	0.841	25.919
Hao et al.	2022	107.541	-12.426	0.847	-3.02	0.835	–

💡 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	–	1.01	–	16	0.414	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CMa08	100.0	107.43	-12.28	0.86	-3.15	0.88	26.44	0.5
CWWDL 14345	48.3	107.43	-12.14	0.87	-3.2	0.92	22.81	0.01

💡 Note: The % column shows the percentage of members that OC 0379 shares with each listed object.

Visualization

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