OC 0530

0.22 UTI

0.27

C_N

1.0

C_dens

0.75

C_C3

0.25

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 27

Radius (P>50% members) 1.8 [arcmin]

C_N 0.27 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 0.44 Possibly duplicate

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

Overview

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OC 0530 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly 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. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for OC 0530 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	–	148.286	-57.399	0.342	-5.565	3.683	–
Hunt & Reffert	2024	148.28	-57.402	0.342	-5.543	3.661	–
Cavallo et al.	2024	148.274	-57.415	0.341	–	–	–
Hunt & Reffert	2023	148.28	-57.402	0.342	-5.543	3.661	–
Hao et al.	2022	148.243	-57.398	0.334	-5.546	3.703	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	425*	–	–
Cavallo et al.	2024	2.44	2.11	–	23	0.050	–	–	–
Hunt & Reffert	2023	2.69	1.88	0.66	30	–	–	–	–
Hao et al.	2022	–	1.58	–	32	0.611	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 780	55.6	148.3	-57.41	0.35	-5.56	3.65	–	0.24

💡 Note: The % column shows the percentage of members that OC 0530 shares with each listed object.

Visualization

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