Cep OB6

0.00 UTI

0.25

C_N

0.38

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification BB

C_N 0.25 Poorly populated
C_dens 0.38 Loose
C_C3 0.5 Intermediate 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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Cep OB6 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a 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 Young

Data

🔍 Search references for Cep OB6 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–	335.129	56.437	4.129	16.792	4.786	-14.344
He et al.	2022	334.481	56.35	4.124	16.352	4.81	–

💡 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–	–	0.35	–	63	–	–	–	–
He et al.	2022	–	0.35	–	63	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Delta Cephei Cluster	100.0	335.47	56.64	4.14	16.9	4.72	-14.54	0.5
OCSN 33	100.0	335.08	56.53	4.13	16.79	4.81	-13.98	0.06

💡 Note: The % column shows the percentage of members that Cep OB6 shares with each listed object.

Visualization

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