FSR 0126

(MWSC 3091)

0.30 UTI

0.0

C_N

0.12

C_dens

0.5

C_C3

0.44

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 19

Radius (P>50% members) 6.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.5 Intermediate 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 0126 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.17 kpc) differs significantly from the median photometric distance (~2.11 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for FSR 0126 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	–	290.271	13.7	0.315	-1.609	-4.527	18.897
Just et al.	2023	290.259	13.763	–	–	–	–
Bica et al.	2019	290.287	13.779	–	–	–	–
Kharchenko et al.	2016	290.259	13.763	–	–	–	–
Dias et al.	2014	290.288	13.775	–	2.02	-2.38	–
Kharchenko et al.	2013	290.265	13.765	–	0.92	-6.02	–
Froebrich et al.	2007	290.288	13.775	–	–	–	–
Dias et al.	2002	290.288	13.775	–	2.02	-2.38	–

💡 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	–	–	–	9	–	209	–	–
Kharchenko et al.	2016	2.11	3.65	–	9	–	–	–	–
Kharchenko et al.	2013	2.11	3.65	–	9	–	–	–	–
Dias et al.	2002	2.11	3.65	–	9	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 406	44.0	290.25	13.6	0.32	-1.57	-4.54	24.12	0.04

💡 Note: The % column shows the percentage of members that FSR 0126 shares with each listed object.

Visualization

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