FSR 0129

(MWSC 3123)

0.36 UTI

0.25

C_N

0.55

C_dens

0.25

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 25

Radius (P>50% members) 2.9 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.55 Moderately dense
C_C3 0.25 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0129 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate^* distance, below 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 (~3.56 kpc) differs significantly from the median photometric distance (~1.30 kpc).

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

Relatively close High extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0129 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	–	291.731	13.952	0.281	-3.059	-5.876	59.282
Just et al.	2023	291.736	13.972	–	–	–	–
Bica et al.	2019	291.736	13.988	–	–	–	–
Kharchenko et al.	2016	291.736	13.972	–	–	–	–
Kharchenko et al.	2013	291.742	13.975	–	1.05	-5.0	–
Froebrich et al.	2007	291.733	13.982	–	–	–	–
Dias et al.	2002	291.733	13.982	–	-0.39	0.18	–

💡 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	–	–	–	302	–	18	–	–
Kharchenko et al.	2016	1.30	4.07	–	302	–	–	–	–
Kharchenko et al.	2013	1.30	4.07	–	302	–	–	–	–
Dias et al.	2002	1.30	4.07	–	302	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1700	80.0	291.73	13.95	0.28	-3.07	-5.89	59.28	0.03

💡 Note: The % column shows the percentage of members that FSR 0129 shares with each listed object.

Visualization

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