FSR 1088

0.47 UTI

0.34

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 171.7 [N/pc²]

C3 classification AA

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high 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 1088 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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 large percentage of members with 2 later reported entries. See table with shared members information.

No fundamental parameters

Data

🔍 Search references for FSR 1088 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–	85.266	-9.352	2.288	0.489	-1.201	16.609
Froebrich et al.	2007	85.254	-9.351	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 70	97.1	85.34	-9.45	2.27	0.53	-1.21	16.14	0.32
OC 0356	76.5	85.3	-9.47	2.25	0.56	-1.28	15.99	0.42

💡 Note: The % column shows the percentage of members that FSR 1088 shares with each listed object.

Visualization

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