FSR 0632

(MWSC 285)

0.39 UTI

0.0

C_N

0.1

C_dens

0.62

C_C3

0.62

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 23

Radius (P>50% members) 26.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.62 Moderately studied
C_dup 1.0 Unique

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

Overview

FSR 0632 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Hunt & Reffert (2024): Classified as a moving group.

Cavallo et al. (2024): Gold sample.

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	52.939	59.125	1.137	4.032	-1.704	-0.14
Hu & Soubiran	2025	53.066	59.085	–	–	–	–
Zhang et al.	2024	53.013	59.133	–	–	–	–
Cavallo et al.	2024	53.066	59.085	1.135	–	–	–
Hunt & Reffert	2023	53.013	59.133	1.131	4.008	-1.708	-3.421
Just et al.	2023	53.132	59.208	–	–	–	–
Bica et al.	2019	53.108	59.184	–	–	–	–
Kharchenko et al.	2016	53.132	59.208	–	–	–	–
Kharchenko et al.	2013	53.145	59.21	–	1.87	-2.32	–
Kharchenko et al.	2012	53.145	59.21	–	1.87	-2.32	–
Froebrich et al.	2007	53.108	59.18	–	–	–	–

💡 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
Hu & Soubiran	2025	–	–	–	–	-0.140*	–	–	–
Zhang et al.	2024	–	–	–	–	-0.135*	–	–	–
Cavallo et al.	2024	0.87	0.95	–	676	0.030	–	–	–
Hunt & Reffert	2023	0.84	1.00	0.58	385	–	–	–	–
Just et al.	2023	–	–	–	224	–	52	–	–
Kharchenko et al.	2016	1.04	2.13	–	224	–	–	–	–
Kharchenko et al.	2013	1.04	2.13	–	224	–	–	–	–
Kharchenko et al.	2012	1.04	2.13	–	224	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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💡 Note: How are the galactocentric plots generated? See FAQ.