SAI 82

(MWSC 1366)

0.25 UTI

0.27

C_N

0.09

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 27

Radius (P>50% members) 8.6 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.09 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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SAI 82 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.13 kpc) differs significantly from the median photometric distance (~1.29 kpc).

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for SAI 82 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	–	118.059	-33.089	0.32	-3.732	4.509	24.488
Just et al.	2023	118.051	-33.037	–	–	–	–
Bica et al.	2019	118.06	-33.044	–	–	–	–
Kharchenko et al.	2016	118.051	-33.037	–	–	–	–
Kharchenko et al.	2013	118.056	-33.04	–	-3.58	9.46	–
Glushkova et al.	2010	118.06	-33.041	–	–	–	–
Dias et al.	2002	118.058	-33.041	–	0.42	3.74	–

💡 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	–	–	–	447	–	25	–	–
Kharchenko et al.	2016	1.44	2.06	–	447	–	–	–	–
Kharchenko et al.	2013	1.44	2.06	–	447	–	–	–	–
Glushkova et al.	2010	1.15	1.21	–	447	–	–	–	–
Dias et al.	2002	1.15	1.21	–	447	–	–	–	–

Visualization

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