Kronberger 12

(MWSC 808; DSH J0614.2+2229)

0.57 UTI

0.45

C_N

1.0

C_dens

0.5

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 39.8 [N/pc²]

C3 classification BB

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Kronberger 12 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.66 kpc) differs significantly from the median photometric distance (~1.89 kpc).

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for Kronberger 12 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–	93.567	22.494	0.274	-0.251	-1.201	–
Just et al.	2023	93.553	22.484	–	–	–	–
Bica et al.	2019	93.565	22.501	–	–	–	–
Kharchenko et al.	2016	93.553	22.484	–	–	–	–
Kharchenko et al.	2013	93.562	22.483	–	-1.04	-5.85	–
Bukowiecki et al.	2011	93.567	22.5	–	–	–	–
Kronberger et al.	2006	93.565	22.498	–	–	–	–
Dias et al.	2002	93.562	22.498	–	13.28	-0.72	–

💡 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–	1.89	2.395	–	741	–	202	–	–
Just et al.	2023	–	–	–	741	–	49	–	–
Kharchenko et al.	2016	1.89	2.06	–	741	–	–	–	–
Kharchenko et al.	2013	1.89	2.06	–	741	–	–	–	–
Bukowiecki et al.	2012	–	–	–	–	–	356	–	–
Bukowiecki et al.	2011	3.82⁽¹⁾	2.73	–	22	–	–	–	–
Dias et al.	2002	1.77	3.01	–	158	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2156	51.1	93.56	22.5	0.33	-0.21	-1.17	–	0.02

💡 Note: The % column shows the percentage of members that Kronberger 12 shares with each listed object.

Visualization

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