FSR 0614

(MWSC 224)

0.15 UTI

0.0

C_N

0.06

C_dens

0.25

C_C3

0.23

C_lit

1.0

C_dup

N_m (P>50%) 22

Core radius and density 2.6 [pc], 0.3 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.25 Low 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 0614 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Very young

Data

🔍 Search references for FSR 0614 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	40.653	56.742	0.274	-0.324	-1.052	–
Just et al.	2023	40.608	56.732	–	–	–	–
Bica et al.	2019	40.652	56.735	–	–	–	–
Dias et al.	2018	–	–	–	0.09	-1.3	–
Sampedro et al.	2017	40.642	56.733	–	–	–	–
Kharchenko et al.	2016	40.608	56.732	–	–	–	–
Kharchenko et al.	2013	40.62	56.735	–	0.17	-2.66	–
Kharchenko et al.	2012	40.62	56.735	–	0.19	-2.81	–
Froebrich et al.	2007	40.642	56.733	–	–	–	–
Dias et al.	2002	40.642	56.733	–	0.19	-2.81	–

💡 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–	2.61	2.66	–	6	–	240	–	–
Just et al.	2023	–	–	–	6	–	240	–	–
Kharchenko et al.	2016	2.79	2.69	–	6	–	–	–	–
Kharchenko et al.	2013	2.79	2.69	–	6	–	–	–	–
Kharchenko et al.	2012	2.43	2.63	–	631	–	–	–	–
Dias et al.	2002	2.43	2.63	–	631	–	–	–	–

Visualization

ℹ️