FSR 0133

(SAI 128; MWSC 3130)

0.87 UTI

1.0

C_N

1.0

C_dens

0.75

C_C3

0.81

C_lit

1.0

C_dup

N₅₀ (P>50% members) 615

Stellar density (N₅₀/rad) 33.1 [N/pc²]

C3 classification AB

C_N 1.0 Very rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.81 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

FSR 0133 is a very rich, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by very high extinction. It is catalogued as an extremely massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~4.94 kpc) differs significantly from the median photometric distance (~3.60 kpc).

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

Distant Very high extinction Extremely massive Metal-rich Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

🔍 Search references for FSR 0133 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	292.447	15.559	0.202	-2.407	-4.732	19.527
Hunt & Reffert	2024	292.447	15.56	0.223	-2.409	-4.777	19.411
Cavallo et al.	2024	292.447	15.551	0.235	–	–	–
Hunt & Reffert	2023	292.447	15.56	0.223	-2.409	-4.777	19.411
Just et al.	2023	292.43	15.551	–	–	–	–
Cantat-Gaudin et al.	2020	292.448	15.561	0.099	-2.37	-4.576	–
Cantat-Gaudin & Anders	2020	292.448	15.561	0.099	-2.37	-4.576	–
Soubiran et al.	2018	292.448	15.561	–	–	–	19.37
Bica et al.	2019	292.449	15.571	–	–	–	–
Cantat-Gaudin et al.	2018	292.448	15.561	0.099	-2.37	-4.576	–
Kharchenko et al.	2016	292.43	15.551	–	–	–	–
Dias et al.	2014	292.446	15.574	–	0.77	-3.46	–
Kharchenko et al.	2013	292.437	15.553	–	0.94	-6.51	–
Glushkova et al.	2010	292.445	15.564	–	–	–	–
Froebrich et al.	2007	292.446	15.574	–	–	–	–
Dias et al.	2002	292.446	15.574	–	0.77	-3.46	–

💡 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]	B_frac	BSS
UCC	99999–	3.6	6.78	2.8	260	0.530	10162	–	–
Hunt & Reffert	2024	–	–	–	–	–	17851⁽¹⁾	–	–
Cavallo et al.	2024	3.96	5.50	–	66	0.530	–	–	–
Hunt & Reffert	2023	3.60	6.34	2.80	166	–	–	–	–
Just et al.	2023	–	–	–	260	–	2472	–	–
Cantat-Gaudin & Anders	2020	7.82	–	–	–	–	–	–	–
Soubiran et al.	2018	7.82	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	7.82	–	–	–	–	–	–	–
Kharchenko et al.	2016	2.81	6.78	–	260	–	–	–	–
Kharchenko et al.	2013	2.81	6.78	–	260	–	–	–	–
Glushkova et al.	2010	2.08	7.01	–	224	–	–	–	–
Dias et al.	2002	2.81	6.78	–	260	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0076	4.4	292.43	15.54	0.26	-2.43	-4.77	19.16	0.01

💡 Note: The % column shows the percentage of members that FSR 0133 shares with each listed object.

Visualization

ℹ️

1 2 3