SAI 41

(MWSC 469)

0.20 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 13

Radius (P>50% members) 7.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very 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

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SAI 41 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.54 kpc) differs significantly from the median photometric distance (~3.72 kpc).

Distant Moderate extinction Old

Data

🔍 Search references for SAI 41 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	–	76.788	38.42	0.18	0.234	-0.454	-20.945
Just et al.	2023	76.805	38.41	–	–	–	–
Bica et al.	2019	76.776	38.421	–	–	–	–
Kharchenko et al.	2016	76.805	38.41	–	–	–	–
Kharchenko et al.	2013	76.815	38.41	–	-2.68	-2.17	–
Kharchenko et al.	2012	76.815	38.41	–	-2.68	-2.17	–
Glushkova et al.	2010	76.772	38.418	–	–	–	–
Dias et al.	2002	76.771	38.418	–	-2.68	-2.17	–

💡 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	–	–	–	3162	–	79	–	–
Kharchenko et al.	2016	3.72	1.42	–	3162	–	–	–	–
Kharchenko et al.	2013	3.72	1.42	–	3162	–	–	–	–
Kharchenko et al.	2012	3.72	1.42	–	3162	–	–	–	–
Glushkova et al.	2010	5.20	1.58	–	1995	–	–	–	–
Dias et al.	2002	5.20	1.58	–	1995	–	–	–	–

Visualization

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