Teutsch 133

0.12 UTI

0.39

C_N

0.11

C_dens

0.12

C_C3

0.0

C_lit

0.97

C_dup

N₅₀ (P>50% members) 39

Stellar density (N₅₀/rad) 0.6 [N/pc²]

C3 classification DC

C_N 0.39 Poorly populated
C_dens 0.11 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.97 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Teutsch 133 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate 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.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.97) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02. Analysis of Dolidze objects by M. Kronberger reported in DAML02.

Data

🔍 Search references for Teutsch 133 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–	82.476	33.518	0.31	-0.141	-1.591	13.373
Kronberger et al.	2006	82.523	33.488	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
AFGL5142	2.6	82.68	33.85	0.3	0.04	-1.71	34.5	0.04
CWNU 4116	2.6	82.5	33.44	0.45	0.21	-1.93	9.73	0.08
SAI 51	2.6	82.51	33.43	0.45	0.3	-1.95	9.56	0.38

💡 Note: The % column shows the percentage of members that Teutsch 133 shares with each listed object.

Visualization

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