OC 0375

0.27 UTI

0.34

C_N

0.9

C_dens

0.75

C_C3

0.0

C_lit

0.68

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 4.5 [N/pc²]

C3 classification AB

C_N 0.34 Poorly populated
C_dens 0.9 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.68 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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OC 0375 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

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

Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for OC 0375 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–	106.757	-9.174	0.37	-1.174	0.91	–
Hao et al.	2022	106.756	-9.176	0.376	-1.182	0.868	–

💡 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–	–	1.7	–	20	0.223	–	–	–
Hao et al.	2022	–	1.70	–	20	0.223	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1774	70.6	106.74	-9.17	0.37	-1.17	0.91	–	0.01
UBC 218	32.4	106.52	-9.18	0.35	-1.18	0.89	–	0.16
CWWDL 4703	5.9	106.42	-9.12	0.35	-1.09	0.89	–	0.08

💡 Note: The % column shows the percentage of members that OC 0375 shares with each listed object.

Visualization

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