OC 0097

0.00 UTI

0.27

C_N

0.82

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 27

Stellar density (N₅₀/rad) 4.1 [N/pc²]

C3 classification AA

C_N 0.27 Poorly populated
C_dens 0.82 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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OC 0097 is a poorly populated, dense object of very high 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, 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. See table with shared members information.

Low extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0097 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	99999–	299.831	33.741	0.261	-3.514	-6.457	–
Hao et al.	2022	299.839	33.751	0.275	-3.505	-6.476	–

💡 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]	B_frac	BSS
UCC	99999–	–	0.34	–	2	0.112	–	–	–
Hao et al.	2022	–	0.34	–	2	0.112	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 135	100.0	299.82	33.73	0.24	-3.51	-6.44	2.12	0.69

💡 Note: The % column shows the percentage of members that OC 0097 shares with each listed object.

Visualization

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