Kronberger 14

0.06 UTI

0.46

C_N

0.5

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

N₅₀ (P>50% members) 46

Stellar density (N₅₀/rad) 2.5 [N/pc²]

C3 classification AA

C_N 0.46 Poorly populated
C_dens 0.5 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Kronberger 14 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a large 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 20 years.

⚠️ Warning: This is 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 Kronberger 14 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–	315.928	47.194	0.149	-3.383	-3.892	-96.774
Kronberger et al.	2006	315.805	47.076	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 156	84.8	315.95	47.22	0.18	-3.39	-3.85	-82.2	0.85

💡 Note: The % column shows the percentage of members that Kronberger 14 shares with each listed object.

Visualization

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