Kronberger 33

0.48 UTI

0.66

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 82

Stellar density (N₅₀/rad) 8.2 [N/pc²]

C3 classification AB

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 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

ℹ️

Kronberger 33 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a very 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 20 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 Kronberger 33 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	143.177	-53.274	0.092	-3.38	3.474	57.237
Kronberger et al.	2006	143.178	-53.277	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1466	76.8	143.18	-53.27	0.09	-3.37	3.48	72.55	0.02

💡 Note: The % column shows the percentage of members that Kronberger 33 shares with each listed object.

Visualization

ℹ️