FSR 1481

(MWSC 1737)

0.18 UTI

0.0

C_N

0.26

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 23

Radius (P>50% members) 6.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.26 Loose
C_C3 0.12 Very 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

ℹ️

FSR 1481 is a sparse, loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.28 kpc) differs significantly from the median photometric distance (~4.10 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.

Distant Moderate extinction Massive Old

Data

🔍 Search references for FSR 1481 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	149.765	-43.908	0.439	-8.848	4.962	–
Just et al.	2023	149.83	-43.904	–	–	–	–
Kharchenko et al.	2016	149.83	-43.904	–	–	–	–
Kharchenko et al.	2013	149.835	-43.908	–	-12.95	3.85	–
Froebrich et al.	2007	149.854	-43.908	–	–	–	–

💡 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	–	–	–	1318	–	2655	–	–
Kharchenko et al.	2016	4.10	1.29	–	1318	–	–	–	–
Kharchenko et al.	2013	4.10	1.29	–	1318	–	–	–	–

Visualization

ℹ️