AFGL6366-S

0.35 UTI

0.26

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 7.8 [N/pc²]

C3 classification BB

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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-S is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

(*): The parallax distance estimate (~2.10 kpc) differs significantly from the median photometric distance (~1.50 kpc).

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.

Relatively close

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

Lada & Lada (2003)
Embedded cluster within ∼2 Kpc of the Sun.

Data

🔍 Search references for AFGL6366-S 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–	92.132	21.518	0.477	0.396	-1.907	–
Lada & Lada	2003	92.17	21.517	–	–	–	–
Bica et al.	2003	92.166	21.517	–	–	–	–

💡 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–	1.5	–	–	–	–	300	–	–
Lada & Lada	2003	1.50	–	–	–	–	300	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gem4	100.0	92.13	21.53	0.47	0.38	-1.91	–	0.31
AFGL6366-N	57.7	92.16	21.54	0.49	0.34	-2.1	–	0.25
DB2001-27	19.2	92.38	21.4	0.52	0.19	-2.35	44.54	0.37

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

Visualization

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