FSR 0416

(MWSC 3689)

0.76 UTI

0.69

C_N

1.0

C_dens

1.0

C_C3

0.56

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 88

Radius (P>50% members) 10.7 [arcmin]

C_N 0.69 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 0416 is a moderately populated, very dense object of very high 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, young cluster (see Parameters). It is moderately studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Close Moderate extinction Near-solar metallicity Young

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	–	345.387	62.989	1.177	-1.002	-2.319	-18.498
Hunt & Reffert	2024	345.478	63.005	1.181	-0.98	-2.352	-46.659
Cavallo et al.	2024	345.431	63.014	1.181	–	–	–
Hunt & Reffert	2023	345.478	63.005	1.181	-0.98	-2.352	-46.659
Just et al.	2023	345.518	63.061	–	–	–	–
Kharchenko et al.	2016	345.518	63.061	–	–	–	–
Kharchenko et al.	2013	345.525	63.065	–	-1.49	-0.09	–
Kharchenko et al.	2012	345.525	63.065	–	-1.49	-0.09	–
Froebrich et al.	2007	345.571	63.063	–	–	–	–
Dias et al.	2002	345.571	63.063	–	-0.05	-1.47	–

💡 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	–	–	–	–	–	101*	–	–
Cavallo et al.	2024	0.84	2.53	–	9	0.200	–	–	–
Hunt & Reffert	2023	0.82	2.33	0.43	5	–	–	–	–
Just et al.	2023	–	–	–	71	–	8	–	–
Kharchenko et al.	2016	0.70	1.71	–	71	–	–	–	–
Kharchenko et al.	2013	0.70	1.71	–	71	–	–	–	–
Kharchenko et al.	2012	0.70	1.71	–	71	–	–	–	–
Dias et al.	2002	0.70	1.71	–	71	–	–	–	–

💡 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.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2249	98.9	344.27	62.76	1.18	-0.95	-2.29	-19.96	0.4

💡 Note: The % column shows the percentage of members that FSR 0416 shares with each listed object.

Visualization

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