Kronberger 68

(MWSC 3220; DSH J2000.6+3035)

0.26 UTI

0.0

C_N

0.04

C_dens

0.25

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 15

Radius (P>50% members) 5.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.25 Low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Kronberger 68 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~5.34 kpc) differs significantly from the median photometric distance (~0.98 kpc).

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

Close Very high extinction Low mass Intermediate age

Data

🔍 Search references for Kronberger 68 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	–	300.151	30.565	0.187	-2.865	-5.479	-9.799
Just et al.	2023	300.145	30.574	–	–	–	–
Bica et al.	2019	300.147	30.588	–	–	–	–
Loktin & Popova	2017	300.15	30.59	–	-2.209	-3.326	–
Kharchenko et al.	2016	300.145	30.574	–	–	–	–
Dias et al.	2014	300.15	30.59	–	-0.42	-2.44	–
Kharchenko et al.	2013	300.15	30.577	–	-3.27	-5.46	–
Kronberger et al.	2006	300.152	30.59	–	–	–	–
Dias et al.	2002	300.15	30.59	–	-3.27	-5.46	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	347	–	18	–	–
Loktin & Popova	2017	2.76	1.98	–	380	–	–	–	–
Kharchenko et al.	2016	0.98	6.26	–	347	–	–	–	–
Kharchenko et al.	2013	0.98	6.26	–	347	–	–	–	–
Dias et al.	2002	0.71	6.79	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3016	28.0	300.14	30.59	0.12	-2.81	-5.56	-17.96	0.06

💡 Note: The % column shows the percentage of members that Kronberger 68 shares with each listed object.

Visualization

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