Kronberger 74

(FSR 0204; MWSC 3304)

0.21 UTI

0.0

C_N

0.16

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 21

Radius (P>50% members) 5.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

Kronberger 74 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.27 kpc) differs significantly from the median photometric distance (~2.40 kpc).

Relatively close Moderate extinction Low mass Old

Data

🔍 Search references for Kronberger 74 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	304.509	36.788	0.306	-2.238	-6.323	-21.644
Just et al.	2023	304.509	36.757	–	–	–	–
Kharchenko et al.	2016	304.509	36.757	–	–	–	–
Kharchenko et al.	2013	304.515	36.76	–	-4.21	-5.64	-14.5
Froebrich et al.	2007	304.442	36.766	–	–	–	–
Kronberger et al.	2006	304.488	36.76	–	–	–	–
Dias et al.	2002	304.488	36.76	–	14.64	20.68	–

💡 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	–	–	–	1000	–	10	–	–
Kharchenko et al.	2016	2.40	2.84	–	1000	–	–	–	–
Kharchenko et al.	2013	2.40	2.84	–	1000	–	–	–	–
Dias et al.	2002	1.76	2.70	–	1000	–	–	–	–

Visualization

ℹ️