Ruprecht 13

(MWSC 1116; OCL 631; ESO 491 17)

0.20 UTI

0.0

C_N

0.0

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 7

Radius (P>50% members) 8.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.0 Very loose
C_C3 0.12 Very low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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Ruprecht 13 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~8.74 kpc) differs significantly from the median photometric distance (~2.28 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for Ruprecht 13 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	–	106.94	-25.827	0.114	-0.912	1.453	–
Just et al.	2023	106.997	-25.878	–	–	–	–
Bica et al.	2019	107.012	-25.86	–	–	–	–
Loktin & Popova	2017	106.98	-25.88	–	-4.093	4.732	–
Kharchenko et al.	2016	106.997	-25.878	–	–	–	–
Dias et al.	2014	106.963	-25.87	–	-2.15	-0.96	–
Kharchenko et al.	2013	107.002	-25.88	–	-5.09	5.58	–
Dias et al.	2002	106.963	-25.87	–	-2.15	-0.96	–

💡 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	–	–	–	776	–	656	–	–
Loktin & Popova	2017	2.97	0.69	–	759	–	–	–	–
Kharchenko et al.	2016	2.28	1.10	–	776	–	–	–	–
Kharchenko et al.	2013	2.28	1.10	–	776	–	–	–	–
Dias et al.	2002	1.30	0.81	–	1000	–	–	–	–

Visualization

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