FSR 1450

(SAI 100; MWSC 1609)

0.60 UTI

0.51

C_N

1.0

C_dens

0.75

C_C3

0.38

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 1.1 [arcmin]

C_N 0.51 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

FSR 1450 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large^* 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.

(*): The parallax distance estimate (~8.73 kpc) differs significantly from the median photometric distance (~1.38 kpc).

Relatively close High extinction Low mass Intermediate age

Data

🔍 Search references for FSR 1450 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	134.559	-46.292	0.115	-3.074	3.638	–
Just et al.	2023	134.597	-46.3	–	–	–	–
Bica et al.	2019	134.557	-46.289	–	–	–	–
Kharchenko et al.	2016	134.597	-46.3	–	–	–	–
Kharchenko et al.	2013	134.602	-46.303	–	-8.43	12.35	–
Glushkova et al.	2010	134.551	-46.289	–	–	–	–
Froebrich et al.	2007	134.575	-46.303	–	–	–	–

💡 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	–	–	–	251	–	45	–	–
Kharchenko et al.	2016	1.38	4.84	–	251	–	–	–	–
Kharchenko et al.	2013	1.38	4.84	–	251	–	–	–	–
Glushkova et al.	2010	5.37	5.02	–	1259	–	–	–	–

Visualization

ℹ️