FSR 1115

(MWSC 739)

0.58 UTI

0.27

C_N

1.0

C_dens

0.75

C_C3

0.44

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 27

Radius (P>50% members) 1.5 [arcmin]

C_N 0.27 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 1115 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Relatively close Very high extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data

🔍 Search references for FSR 1115 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	–	92.058	-9.585	1.175	-2.628	0.975	68.954
Hunt & Reffert	2024	92.056	-9.58	1.173	-2.682	0.934	68.941
Cavallo et al.	2024	91.986	-9.519	1.178	–	–	–
Hunt & Reffert	2023	92.056	-9.58	1.173	-2.682	0.934	68.941
Just et al.	2023	92.049	-9.579	–	–	–	–
Kharchenko et al.	2016	92.049	-9.579	–	–	–	–
Kharchenko et al.	2013	92.055	-9.58	–	0.55	3.41	–
Froebrich et al.	2007	92.067	-9.596	–	–	–	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	94*	–	–
Cavallo et al.	2024	2.58	2.54	–	2399	0.020	–	–	–
Hunt & Reffert	2023	0.82	3.19	2.23	17	–	–	–	–
Just et al.	2023	–	–	–	8	–	32	–	–
Kharchenko et al.	2016	1.07	7.29	–	8	–	–	–	–
Kharchenko et al.	2013	1.07	7.29	–	8	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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