FSR 1415

(SAI 93; MWSC 1526)

0.23 UTI

0.0

C_N

0.01

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 6.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.12 Very low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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FSR 1415 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by very high extinction. It is catalogued as an old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~9.29 kpc) differs significantly from the median photometric distance (~3.50 kpc).

Distant Very high extinction Old

Data

🔍 Search references for FSR 1415 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	–	130.102	-44.719	0.108	-2.483	2.56	73.084
Just et al.	2023	130.09	-44.722	–	–	–	–
Bica et al.	2019	130.096	-44.735	–	–	–	–
Kharchenko et al.	2016	130.09	-44.722	–	–	–	–
Dias et al.	2014	130.092	-44.734	–	0.39	3.56	–
Kharchenko et al.	2013	130.095	-44.725	–	-6.16	4.93	–
Glushkova et al.	2010	130.091	-44.734	–	–	–	–
Froebrich et al.	2007	130.104	-44.736	–	–	–	–
Dias et al.	2002	130.092	-44.734	–	0.39	3.56	–

💡 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	–	–	–	1778	–	223	–	–
Kharchenko et al.	2016	3.47	6.13	–	1778	–	–	–	–
Kharchenko et al.	2013	3.47	6.13	–	1778	–	–	–	–
Glushkova et al.	2010	3.53	5.80	–	1778	–	–	–	–
Dias et al.	2002	3.53	5.80	–	1778	–	–	–	–

Visualization

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