FSR 1351

(MWSC 1331)

0.65 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 114

Radius (P>50% members) 4.3 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 1351 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.69 kpc) differs significantly from the median photometric distance (~1.58 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 Intermediate age

Data

🔍 Search references for FSR 1351 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	–	116.484	-34.34	0.271	-2.09	3.153	–
Just et al.	2023	116.455	-34.337	–	–	–	–
Kharchenko et al.	2016	116.455	-34.337	–	–	–	–
Kharchenko et al.	2013	116.46	-34.34	–	-3.36	4.42	142.0
Froebrich et al.	2007	116.479	-34.341	–	–	–	–

💡 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	–	–	–	158	–	97	–	–
Kharchenko et al.	2016	1.58	2.00	–	158	–	–	–	–
Kharchenko et al.	2013	1.58	2.00	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1352	78.1	116.57	-34.31	0.26	-2.07	3.14	–	0.86
Cmg 1066	57.0	116.57	-34.31	0.27	-2.06	3.17	–	0.0

💡 Note: The % column shows the percentage of members that FSR 1351 shares with each listed object.

Visualization

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