Teutsch 136

(Koposov 82)

0.44 UTI

0.37

C_N

1.0

C_dens

0.75

C_C3

0.03

C_lit

1.0

C_dup

N₅₀ (P>50% members) 37

Stellar density (N₅₀/rad) 123.2 [N/pc²]

C3 classification BA

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.03 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Teutsch 136 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Very young

Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.

Data

🔍 Search references for Teutsch 136 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–	92.988	20.674	0.531	-0.291	-2.435	1.647
Dias et al.	2026	92.981	20.684	0.511	-0.263	-2.349	–
Glushkova et al.	2010	92.983	20.671	–	–	–	–
Kronberger et al.	2006	92.992	20.674	–	–	–	–

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

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	1.86	1.74	–	6	-0.154	–	–	–
Dias et al.	2026	1.86	1.74	–	6	-0.154	–	–	–

Visualization

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