OC 0110

0.03 UTI

0.0

C_N

0.06

C_dens

0.25

C_C3

0.0

C_lit

0.44

C_dup

C3 classification DB

Number of members (P>50%) 18

Radius (P>50% members) 14.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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OC 0110 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a small percentage 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 0110 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	–	306.025	36.233	0.532	-2.374	-4.371	16.24
Hao et al.	2022	306.086	36.263	0.526	-2.337	-4.373	–

💡 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]	Bfr	BSS
Hao et al.	2022	–	0.24	–	10	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 371	56.0	305.89	36.08	0.52	-2.39	-4.37	-25.38	0.37
OC 0108	24.0	305.93	35.92	0.54	-2.39	-4.51	–	0.14

💡 Note: The % column shows the percentage of members that OC 0110 shares with each listed object.

Visualization

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