OC 0613

0.42 UTI

0.31

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.9

C_dup

C3 classification AA

Number of members (P>50%) 31

Radius (P>50% members) 1.3 [arcmin]

C_N 0.31 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.9 Very likely unique

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

Overview

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OC 0613 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

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

Moderate extinction Metal-rich Young

Data

🔍 Search references for OC 0613 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	–	219.786	-61.081	0.181	-5.296	-3.072	51.065
Hao et al.	2022	219.795	-61.082	0.173	-5.326	-3.117	–

💡 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	–	1.06	–	63	0.537	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1174	9.7	219.48	-61.12	0.28	-5.28	-2.93	-70.43	0.06

💡 Note: The % column shows the percentage of members that OC 0613 shares with each listed object.

Visualization

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