FSR 1065

(MWSC 925)

0.23 UTI

0.0

C_N

0.02

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 11

Radius (P>50% members) 6.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.25 Low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 1065 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* 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 (~5.80 kpc) differs significantly from the median photometric distance (~1.55 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for FSR 1065 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	–	99.043	-0.684	0.172	-0.487	0.31	62.703
Just et al.	2023	99.013	-0.665	–	–	–	–
Bica et al.	2019	98.997	-0.663	–	–	–	–
Kharchenko et al.	2016	99.013	-0.665	–	–	–	–
Dias et al.	2014	98.996	-0.668	–	-1.1	1.63	–
Kharchenko et al.	2013	99.019	-0.667	–	1.06	-1.19	–
Froebrich et al.	2007	98.996	-0.668	–	–	–	–
Dias et al.	2002	98.996	-0.668	–	1.06	-1.19	–

💡 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	–	–	–	617	–	53	–	–
Kharchenko et al.	2016	1.55	1.42	–	617	–	–	–	–
Kharchenko et al.	2013	1.55	1.42	–	617	–	–	–	–
Dias et al.	2002	1.55	1.42	–	617	–	–	–	–

Visualization

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