FSR 0188

(MWSC 3228)

0.60 UTI

0.64

C_N

0.79

C_dens

0.75

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 78

Stellar density (N₅₀/rad) 3.9 [N/pc²]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 0.79 Dense
C_C3 0.75 High quality
C_lit 0.4 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0188 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.95 kpc) differs significantly from the median photometric distance (~3.35 kpc).

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

Distant High extinction Intermediate age

Data

🔍 Search references for FSR 0188 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	99999–	300.527	33.912	0.144	-2.34	-4.884	10.03
Just et al.	2023	300.489	33.915	–	–	–	–
Bica et al.	2019	300.525	33.922	–	–	–	–
Kharchenko et al.	2016	300.489	33.915	–	–	–	–
Dias et al.	2014	300.521	33.919	–	-1.14	-5.43	–
Kharchenko et al.	2013	300.495	33.917	–	-4.04	-3.14	–
Froebrich et al.	2007	300.521	33.919	–	–	–	–
Dias et al.	2002	300.521	33.919	–	-1.14	-5.43	–

💡 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–	3.35	4.07	–	158	–	279	–	–
Just et al.	2023	–	–	–	158	–	279	–	–
Kharchenko et al.	2016	3.35	4.07	–	158	–	–	–	–
Kharchenko et al.	2013	3.35	4.07	–	158	–	–	–	–
Dias et al.	2002	3.35	4.07	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3359	84.6	300.53	33.91	0.14	-2.32	-4.88	8.38	0.29

💡 Note: The % column shows the percentage of members that FSR 0188 shares with each listed object.

Visualization

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