Ruprecht 11

(MWSC 1108; OCL 607; ESO 558 12)

0.23 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 14

Radius (P>50% members) 8.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 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 11 is a sparse, very loose object of 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 (~7.10 kpc) differs significantly from the median photometric distance (~1.96 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for Ruprecht 11 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	–	106.891	-20.758	0.141	-1.134	2.041	–
Just et al.	2023	106.837	-20.793	–	–	–	–
Bica et al.	2019	106.84	-20.78	–	–	–	–
Loktin & Popova	2017	106.845	-20.795	–	-0.717	2.224	–
Kharchenko et al.	2016	106.837	-20.793	–	–	–	–
Dias et al.	2014	106.838	-20.8	–	-0.71	2.0	–
Kharchenko et al.	2013	106.842	-20.795	–	0.36	-1.12	–
Dias et al.	2002	106.838	-20.8	–	-0.71	2.0	–

💡 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	–	–	–	631	–	131	–	–
Loktin & Popova	2017	2.55	0.30	–	977	–	–	–	–
Kharchenko et al.	2016	1.96	1.35	–	631	–	–	–	–
Kharchenko et al.	2013	1.96	1.35	–	631	–	–	–	–
Dias et al.	2002	1.87	0.53	–	1514	–	–	–	–

Visualization

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