FSR 1695

(MWSC 2231)

0.14 UTI

0.31

C_N

0.03

C_dens

0.25

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 31

Core radius and density 4.7 [pc], 0.2 [pc^-2]

C3 classification CC

C_N 0.31 Poorly populated
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 1695 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.61 kpc) differs significantly from the median photometric distance (~1.67 kpc).

⚠️ 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 Low extinction Old

Data

🔍 Search references for FSR 1695 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	99999–	218.408	-49.15	0.277	-8.087	-0.997	–
Bica et al.	2019	218.407	-49.168	–	–	–	–
Dib et al.	2018	218.409	-49.165	–	–	–	–
Joshi et al.	2016	218.409	-49.165	–	–	–	–
Froebrich et al.	2007	218.408	-49.169	–	–	–	–

💡 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–	1.67	0.89	–	2399	–	–	–	–
Dib et al.	2018	1.67	–	–	2399	–	–	–	–
Joshi et al.	2016	1.67	0.89	–	2399	–	–	–	–

Visualization

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