FSR 1651

(MWSC 2118)

0.26 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 10

Radius (P>50% members) 7.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

ℹ️

FSR 1651 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, old cluster (see Parameters). It is moderately studied in the literature.

Distant Moderate extinction Massive Old

Data

🔍 Search references for FSR 1651 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	201.441	-59.0	0.296	-6.996	-1.604	-15.827
Just et al.	2023	201.371	-58.982	–	–	–	–
Sánchez et al.	2020	201.358	-58.972	–	-7.365	-1.284	–
Bica et al.	2019	201.359	-58.972	–	–	–	–
Kharchenko et al.	2016	201.371	-58.982	–	–	–	–
Dias et al.	2014	201.358	-58.972	–	-10.42	-4.14	–
Kharchenko et al.	2013	201.382	-58.985	–	-9.55	3.08	–
Froebrich et al.	2007	201.358	-58.972	–	–	–	–
Dias et al.	2002	201.358	-58.972	–	-10.42	-4.14	–

💡 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	–	–	–	2512	–	4688	–	–
Kharchenko et al.	2016	3.60	1.13	–	2512	–	–	–	–
Kharchenko et al.	2013	3.60	1.13	–	2512	–	–	–	–
Dias et al.	2002	3.60	1.13	–	2512	–	–	–	–

Visualization

ℹ️