FSR 0790

0.01 UTI

0.79

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.02

C_dup

N₅₀ (P>50% members) 200

Stellar density (N₅₀/rad) 5.2 [N/pc²]

C3 classification AB

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0790 is a rich, very dense object of high C3 quality. Its parallax locates it at a large 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.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

No fundamental parameters

Data

🔍 Search references for FSR 0790 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–	76.78	30.854	0.179	0.713	-0.733	-6.699
Froebrich et al.	2007	76.763	30.845	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Skiff J0507+30.8	98.0	76.78	30.85	0.18	0.73	-0.73	-6.72	0.91

💡 Note: The % column shows the percentage of members that FSR 0790 shares with each listed object.

Visualization

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