FSR 0365

(MWSC 3636)

0.23 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 16

Radius (P>50% members) 5.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 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 0365 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 (~6.42 kpc) differs significantly from the median photometric distance (~3.86 kpc).

Distant Moderate extinction Intermediate age

Data

🔍 Search references for FSR 0365 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	–	338.266	55.541	0.156	-1.266	-0.98	–
Just et al.	2023	338.261	55.531	–	–	–	–
Bica et al.	2019	338.291	55.538	–	–	–	–
Kharchenko et al.	2016	338.261	55.531	–	–	–	–
Kharchenko et al.	2013	338.266	55.535	–	-2.59	-2.17	–
Kharchenko et al.	2012	338.266	55.535	–	-2.59	-2.17	–
Froebrich et al.	2007	338.267	55.539	–	–	–	–
Dias et al.	2002	338.267	55.539	–	-3.04	-1.34	–

💡 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	–	–	–	804	–	482	–	–
Kharchenko et al.	2016	3.86	2.55	–	804	–	–	–	–
Kharchenko et al.	2013	3.86	2.55	–	804	–	–	–	–
Kharchenko et al.	2012	3.86	2.55	–	804	–	–	–	–
Dias et al.	2002	3.86	2.55	–	804	–	–	–	–

Visualization

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