Kronberger 55

(MWSC 3772)

0.36 UTI

0.35

C_N

0.3

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 35

Radius (P>50% members) 5.2 [arcmin]

C_N 0.35 Poorly populated
C_dens 0.3 Loose
C_C3 0.38 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 55 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.17 kpc) differs significantly from the median photometric distance (~1.79 kpc).

Relatively close Moderate extinction Low mass Young

Data

🔍 Search references for Kronberger 55 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	358.25	62.771	0.315	-3.057	-1.063	-60.799
Just et al.	2023	358.259	62.774	–	–	–	–
Kharchenko et al.	2016	358.259	62.774	–	–	–	–
Kharchenko et al.	2013	358.267	62.778	–	-1.32	-4.55	–
Kharchenko et al.	2012	358.267	62.778	–	-1.47	-5.31	–
Kronberger et al.	2006	358.29	62.787	–	–	–	–
Dias et al.	2002	358.288	62.787	–	-2.14	-4.54	–

💡 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	–	–	–	24	–	2	–	–
Kharchenko et al.	2016	1.99	2.97	–	24	–	–	–	–
Kharchenko et al.	2013	1.99	2.97	–	24	–	–	–	–
Kharchenko et al.	2012	1.60	2.79	–	62	–	–	–	–
Dias et al.	2002	1.26	3.50	–	398	–	–	–	–

Visualization

ℹ️