OC 0415

0.04 UTI

0.0

C_N

0.31

C_dens

0.5

C_C3

0.0

C_lit

0.24

C_dup

C3 classification BB

Number of members (P>50%) 22

Radius (P>50% members) 4.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.31 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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OC 0415 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Low extinction Near-solar metallicity Old

Data

🔍 Search references for OC 0415 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	–	118.367	-22.403	0.318	-2.243	2.094	47.058
Hao et al.	2022	118.362	-22.389	0.34	-2.179	2.049	107.558

💡 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	–	0.89	–	1259	0.498	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 228	76.0	118.37	-22.4	0.33	-2.26	2.13	47.22	0.44

💡 Note: The % column shows the percentage of members that OC 0415 shares with each listed object.

Visualization

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