FSR 1155

(BDS2003 93)

0.45 UTI

0.61

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 72

Stellar density (N₅₀/rad) 51.7 [N/pc²]

C3 classification AC

C_N 0.61 Moderately 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 1155 is a moderately 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 large percentage of members with a later reported entry. See table with shared members information.

No fundamental parameters

Data

🔍 Search references for FSR 1155 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–	104.3	-8.205	0.764	-2.463	1.101	35.961
Froebrich et al.	2007	104.3	-8.187	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
BDSB 93	87.5	104.3	-8.22	0.75	-2.45	1.12	23.38	0.21

💡 Note: The % column shows the percentage of members that FSR 1155 shares with each listed object.

Visualization

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