FSR 1190

0.38 UTI

0.28

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 28

Stellar density (N₅₀/rad) 30.3 [N/pc²]

C3 classification AC

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 1190 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 19 years.

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

No fundamental parameters

Data

🔍 Search references for FSR 1190 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–	106.745	-11.321	0.847	-4.206	1.443	23.047
Froebrich et al.	2007	106.763	-11.338	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14341	3.6	106.46	-11.12	0.85	-3.92	1.46	22.47	0.12

💡 Note: The % column shows the percentage of members that FSR 1190 shares with each listed object.

Visualization

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