NGC 6775

(MWSC 3079)

0.23 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 11

Radius (P>50% members) 7.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

NGC 6775 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.31 kpc) differs significantly from the median photometric distance (~2.00 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for NGC 6775 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	289.261	-0.958	0.159	-2.863	-5.667	60.877
Just et al.	2023	289.193	-0.924	–	–	–	–
Bica et al.	2019	289.221	-0.92	–	–	–	–
Loktin & Popova	2017	289.245	-0.922	–	2.521	-8.672	–
Kharchenko et al.	2016	289.193	-0.924	–	–	–	–
Dias et al.	2014	289.2	-0.923	–	0.19	-3.6	–
Kharchenko et al.	2013	289.2	-0.922	–	2.28	-7.45	–
Dias et al.	2002	289.2	-0.923	–	2.28	-7.45	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	708	–	245	–	–
Loktin & Popova	2017	2.63	0.80	–	1549	–	–	–	–
Kharchenko et al.	2016	2.00	1.35	–	708	–	–	–	–
Kharchenko et al.	2013	2.00	1.35	–	708	–	–	–	–
Dias et al.	2002	1.19	1.49	–	891	–	–	–	–

Visualization

ℹ️