FSR 0568

(MWSC 201)

0.47 UTI

0.0

C_N

0.99

C_dens

0.62

C_C3

0.38

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 22

Radius (P>50% members) 7.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.99 Very dense
C_C3 0.62 Intermediate 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 0568 is a sparse, very dense 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 an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~0.93 kpc) differs significantly from the median photometric distance (~2.30 kpc).

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Moderate extinction Old

Data

🔍 Search references for FSR 0568 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	–	37.289	72.18	1.074	-1.647	-1.991	-24.864
Just et al.	2023	37.213	72.188	–	–	–	–
Bica et al.	2019	37.266	72.197	–	–	–	–
Kharchenko et al.	2016	37.213	72.188	–	–	–	–
Kharchenko et al.	2013	37.23	72.19	–	-2.46	0.28	–
Kharchenko et al.	2012	37.23	72.19	–	-2.46	0.28	–
Froebrich et al.	2007	37.279	72.197	–	–	–	–

💡 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	–	–	–	1000	–	237	–	–
Kharchenko et al.	2016	2.30	2.98	–	1000	–	–	–	–
Kharchenko et al.	2013	2.30	2.98	–	1000	–	–	–	–
Kharchenko et al.	2012	2.30	2.98	–	1000	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0569	100.0	37.79	72.45	1.08	-1.62	-1.78	-24.86	0.74
UBC 187	56.0	37.86	72.42	1.08	-1.67	-1.74	-24.91	0.0

💡 Note: The % column shows the percentage of members that FSR 0568 shares with each listed object.

Visualization

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