NGC 6595

0.16 UTI

0.0

C_N

0.3

C_dens

0.12

C_C3

0.19

C_lit

1.0

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification CD

C_N 0.0 Sparse
C_dens 0.3 Loose
C_C3 0.12 Very low quality
C_lit 0.19 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 6595 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

⚠️ 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.

Relatively close Moderate extinction Intermediate age

Bica et al. (2019)
2MASS website.

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

Data

🔍 Search references for NGC 6595 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–	274.252	-19.927	0.665	2.561	-3.046	25.047
Sampedro et al.	2017	274.267	-19.865	1.26	-6.16	–	–
Tadross	2014	274.267	-19.865	–	–	–	–
Dias et al.	2014	274.267	-19.865	–	2.73	-3.26	–
Bukowiecki et al.	2011	274.271	-19.869	–	–	–	–
Bica et al.	2003	274.263	-19.866	–	–	–	–
Dias et al.	2002	274.267	-19.865	–	2.73	-3.26	–
Lynga	1987	274.229	-19.883	–	–	–	–
Sulentic et al.	1973	274.246	-19.874	–	–	–	–

💡 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–	1.64	2.97	–	448	–	–	–	–
Tadross	2014	1.64	2.97	–	450	–	–	–	–
Dias et al.	2002	1.64	2.97	–	447	–	–	–	–

Visualization

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