FSR 0265

(MWSC 3484)

0.33 UTI

0.46

C_N

0.44

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 46

Radius (P>50% members) 6.7 [arcmin]

C_N 0.46 Poorly populated
C_dens 0.44 Loose
C_C3 0.25 Low 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 0265 is a poorly populated, 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 an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.35 kpc) differs significantly from the median photometric distance (~1.48 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 Moderate extinction Old

Data

🔍 Search references for FSR 0265 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	–	318.194	41.987	0.425	-5.33	-5.731	–
Just et al.	2023	318.197	41.997	–	–	–	–
Kharchenko et al.	2016	318.197	41.997	–	–	–	–
Kharchenko et al.	2013	318.202	42.0	–	-3.77	1.29	–
Froebrich et al.	2007	318.204	42.01	–	–	–	–

💡 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	–	55	–	–
Kharchenko et al.	2016	1.48	2.45	–	1000	–	–	–	–
Kharchenko et al.	2013	1.48	2.45	–	1000	–	–	–	–

Visualization

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