NGC 6832

0.31 UTI

0.72

C_N

0.05

C_dens

0.62

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 95

Core radius and density 2.4 [pc], 0.3 [pc^-2]

C3 classification AC

C_N 0.72 Moderately populated
C_dens 0.05 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

NGC 6832 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

(*): The parallax distance estimate (~5.70 kpc) differs significantly from the median photometric distance (~1.75 kpc).

Relatively close Low extinction Old

Data

🔍 Search references for NGC 6832 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	296.999	59.38	0.175	-2.104	-2.751	-32.771
Sampedro et al.	2017	297.062	59.422	–	-1.01	-2.78	–
Tadross	2014	297.062	59.422	–	–	–	–
Dias et al.	2014	297.062	59.422	–	-1.17	-2.94	–
Dias et al.	2002	297.062	59.422	–	-1.17	-2.94	–

💡 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–	1.75	0.32	–	3010	–	–	–	–
Tadross	2014	1.75	0.32	–	3000	–	–	–	–
Dias et al.	2002	1.75	0.32	–	3020	–	–	–	–

Visualization

ℹ️