SAI 88

(MWSC 1453)

0.59 UTI

0.68

C_N

1.0

C_dens

0.38

C_C3

0.44

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 86

Radius (P>50% members) 1.7 [arcmin]

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 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 88 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Very distant High extinction Intermediate age

Data

🔍 Search references for SAI 88 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	–	123.244	-41.877	0.161	-1.145	3.31	70.376
He et al.	2023	123.245	-41.875	0.127	-1.135	3.319	–
Just et al.	2023	123.236	-41.872	–	–	–	–
Bica et al.	2019	123.233	-41.886	–	–	–	–
Kharchenko et al.	2016	123.236	-41.872	–	–	–	–
Kharchenko et al.	2013	123.241	-41.875	–	-3.95	4.95	–
Glushkova et al.	2010	123.24	-41.884	–	–	–	–
Dias et al.	2002	123.242	-41.884	–	-3.95	4.95	–

💡 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
He et al.	2023	5.37	3.55	–	1995	–	–	–	–
Just et al.	2023	–	–	–	841	–	762	–	–
Kharchenko et al.	2016	5.84	3.55	–	841	–	–	–	–
Kharchenko et al.	2013	5.84	3.55	–	841	–	–	–	–
Glushkova et al.	2010	8.24	2.85	–	1000	–	–	–	–
Dias et al.	2002	8.24	2.85	–	1000	–	–	–	–

Visualization

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