AFGL6366-N

0.09 UTI

0.0

C_N

0.19

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 23

Core radius and density 2.1 [pc], 1.0 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.19 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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AFGL6366-N is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for AFGL6366-N 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–	92.158	21.541	0.49	0.34	-2.099	–
Bica et al.	2003	92.189	21.54	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gem4	88.0	92.13	21.53	0.47	0.38	-1.91	–	0.25
AFGL6366-S	60.0	92.13	21.52	0.48	0.4	-1.91	–	0.21
DB2001-27	36.0	92.38	21.4	0.52	0.19	-2.35	44.54	0.28
AFGL5180	4.0	92.18	21.68	0.36	-0.07	-1.48	30.87	0.06

💡 Note: The % column shows the percentage of members that AFGL6366-N shares with each listed object.

Visualization

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