Ruprecht 113

(MWSC 2337; OCL 940; ESO 136 09)

0.27 UTI

0.0

C_N

0.09

C_dens

0.25

C_C3

0.5

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 15

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

C_N 0.0 Sparse
C_dens 0.09 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

ℹ️

Ruprecht 113 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.79 kpc) differs significantly from the median photometric distance (~0.81 kpc).

Close Low extinction Intermediate age

Data

🔍 Search references for Ruprecht 113 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	239.375	-59.466	0.264	-5.146	-4.685	–
Bica et al.	2019	239.294	-59.461	–	–	–	–
Kharchenko et al.	2016	239.372	-59.494	–	–	–	–
Dias et al.	2014	239.262	-59.467	–	-5.57	-2.63	–
Kharchenko et al.	2013	239.385	-59.495	–	-3.05	-2.0	–
Piskunov et al.	2008	239.36	-59.485	–	–	–	–
Kharchenko et al.	2005	239.37	-59.49	–	-3.04	-2.1	–
Kharchenko et al.	2003	239.41	-59.43	–	-3.38	-1.34	–
Dias et al.	2002	239.262	-59.467	–	-5.57	-2.63	–

💡 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
Kharchenko et al.	2016	0.81	0.46	–	221	–	–	–	–
Kharchenko et al.	2013	0.81	0.46	–	221	–	–	–	–
Piskunov et al.	2008	0.81	0.46	–	170	–	–	–	–
Kharchenko et al.	2005	0.81	0.46	–	170	–	–	–	–
Kharchenko et al.	2003	0.67	0.31	–	–	–	–	–	–
Dias et al.	2002	0.81	0.46	–	170	–	–	–	–

Visualization

ℹ️