FSR 0245

(MWSC 3382)

0.52 UTI

0.0

C_N

1.0

C_dens

1.0

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 21

Stellar density (N₅₀/rad) 7.0 [N/pc²]

C3 classification AA

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.3 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0245 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0245 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–	309.692	42.149	0.687	-1.909	-3.609	21.616
Just et al.	2023	309.52	42.222	–	–	–	–
Kharchenko et al.	2016	309.52	42.222	–	–	–	–
Kharchenko et al.	2013	309.525	42.225	–	1.98	0.76	–
Froebrich et al.	2007	309.521	42.231	–	–	–	–
Dias et al.	2002	309.521	42.231	–	1.98	0.76	–

💡 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–	1.19	4.13	–	380	–	10	–	–
Just et al.	2023	–	–	–	380	–	10	–	–
Kharchenko et al.	2016	1.19	4.13	–	380	–	–	–	–
Kharchenko et al.	2013	1.19	4.13	–	380	–	–	–	–
Dias et al.	2002	1.19	4.13	–	380	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 640	100.0	309.74	42.15	0.68	-2.32	-3.43	1.13	0.48
DB2001 16	32.0	309.65	42.11	0.69	-2.53	-3.27	114.81	0.44

💡 Note: The % column shows the percentage of members that FSR 0245 shares with each listed object.

Visualization

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