OC 0526

0.00 UTI

0.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 19

Radius (P>50% members) 1.0 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 1.0 Very high 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

ℹ️

OC 0526 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

High extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0526 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	147.322	-54.612	0.255	-4.638	2.873	–
Hao et al.	2022	147.292	-54.611	0.255	-4.65	2.869	–

💡 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	–	3.74	–	5	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 83	100.0	147.31	-54.61	0.25	-4.61	2.89	25.15	0.96
OC 0527	68.0	147.32	-54.61	0.26	-4.61	2.88	–	0.0
OC 0525	40.0	147.31	-54.6	0.22	-4.6	2.87	–	0.0
OC 0528	20.0	147.31	-54.62	0.29	-4.6	2.92	25.6	0.0

💡 Note: The % column shows the percentage of members that OC 0526 shares with each listed object.

Visualization

ℹ️