FSR 0486

(MWSC 32)

0.35 UTI

0.68

C_N

0.0

C_dens

0.62

C_C3

0.23

C_lit

1.0

C_dup

N_m (P>50%) 85

Core radius and density 29 [pc], 0.01 [pc^-2]

C3 classification AC

C_N 0.68 Moderately populated
C_dens 0.0 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.23 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

FSR 0486 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~98.04 kpc) differs significantly from the median photometric distance (~1.85 kpc).

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0486 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	5.092	59.303	0.01	0.014	-0.124	–
Just et al.	2023	5.094	59.329	–	–	–	–
Sánchez et al.	2020	5.088	59.318	–	0.119	-0.056	–
Dias et al.	2018	–	–	–	-1.11	0.42	–
Sampedro et al.	2017	5.088	59.318	–	1.05	-1.41	–
Kharchenko et al.	2016	5.094	59.329	–	–	–	–
Kharchenko et al.	2013	5.103	59.332	–	-2.35	-1.46	–
Kharchenko et al.	2012	5.103	59.332	–	-2.1	-2.11	–
Froebrich et al.	2007	5.088	59.318	–	–	–	–
Dias et al.	2002	5.088	59.318	–	-2.1	-2.11	–

💡 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–	1.85	1.74	–	794	–	7	–	–
Just et al.	2023	–	–	–	794	–	7	–	–
Kharchenko et al.	2016	1.85	1.74	–	794	–	–	–	–
Kharchenko et al.	2013	1.85	1.74	–	794	–	–	–	–
Kharchenko et al.	2012	1.85	1.74	–	794	–	–	–	–
Dias et al.	2002	1.85	1.74	–	794	–	–	–	–

Visualization

ℹ️