FSR 0435

(MWSC 3736)

0.44 UTI

0.31

C_N

0.27

C_dens

0.5

C_C3

0.56

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 31

Radius (P>50% members) 16.6 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.27 Loose
C_C3 0.5 Intermediate quality
C_lit 0.56 Moderately studied
C_dup 1.0 Unique

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

Overview

FSR 0435 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

Close Moderate extinction Low mass Near-solar metallicity Intermediate age

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	–	352.883	59.792	1.009	-1.077	-2.034	-20.872
Hunt & Reffert	2024	352.882	59.78	0.995	-1.051	-2.016	-15.436
Cavallo et al.	2024	352.926	59.811	0.998	–	–	–
Hunt & Reffert	2023	352.882	59.78	0.995	-1.051	-2.016	-15.436
Just et al.	2023	352.799	59.771	–	–	–	–
Kharchenko et al.	2016	352.799	59.771	–	–	–	–
Kharchenko et al.	2013	352.807	59.775	–	-2.33	-0.71	–
Kharchenko et al.	2012	352.807	59.775	–	-2.33	-0.71	–
Froebrich et al.	2007	352.792	59.786	–	–	–	–
Dias et al.	2002	352.792	59.786	–	-2.33	-0.71	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	56*	–	–
Cavallo et al.	2024	1.06	2.28	–	30	0.090	–	–	–
Hunt & Reffert	2023	0.95	2.02	1.01	58	–	–	–	–
Just et al.	2023	–	–	–	224	–	18	–	–
Kharchenko et al.	2016	0.81	1.65	–	224	–	–	–	–
Kharchenko et al.	2013	0.81	1.65	–	224	–	–	–	–
Kharchenko et al.	2012	0.81	1.65	–	224	–	–	–	–
Dias et al.	2002	0.81	1.65	–	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.