FSR 0413

(MWSC 3687)

0.38 UTI

0.0

C_N

1.0

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 21

Radius (P>50% members) 6.7 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0413 is a sparse, very dense object of very low C3 quality. Its parallax locates it at a close^* distance, above the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~0.96 kpc) differs significantly from the median photometric distance (~1.80 kpc).

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

Relatively close High extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0413 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	345.141	62.891	1.046	-2.239	-2.563	2.423
Just et al.	2023	345.202	62.884	–	–	–	–
Kharchenko et al.	2016	345.202	62.884	–	–	–	–
Kharchenko et al.	2013	345.21	62.888	–	-4.95	-2.17	–
Kharchenko et al.	2012	345.21	62.888	–	-4.95	-2.17	–
Froebrich et al.	2007	345.25	62.894	–	–	–	–
Dias et al.	2002	345.25	62.894	–	-4.95	-2.17	–

💡 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	–	–	–	178	–	6	–	–
Kharchenko et al.	2016	1.80	4.80	–	178	–	–	–	–
Kharchenko et al.	2013	1.80	4.80	–	178	–	–	–	–
Kharchenko et al.	2012	1.80	4.80	–	178	–	–	–	–
Dias et al.	2002	1.80	4.80	–	178	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 4	24.0	344.35	62.99	1.16	-2.4	-2.56	-13.56	0.47

💡 Note: The % column shows the percentage of members that FSR 0413 shares with each listed object.

Visualization

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