Ruprecht 95

(MWSC 1966; OCL 863; ESO 129 30)

0.23 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 8

Radius (P>50% members) 8.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very 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

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Ruprecht 95 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.08 kpc) differs significantly from the median photometric distance (~1.63 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for Ruprecht 95 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	–	175.872	-61.136	0.164	-6.336	1.307	-5.39
Just et al.	2023	175.905	-61.151	–	–	–	–
Bica et al.	2019	175.884	-61.139	–	–	–	–
Kharchenko et al.	2016	175.905	-61.151	–	–	–	–
Dias et al.	2014	175.908	-61.133	–	-0.82	-4.0	–
Kharchenko et al.	2013	175.912	-61.155	–	-4.87	-3.99	–
Dias et al.	2002	175.908	-61.133	–	-0.82	-4.0	–

💡 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	–	–	–	313	–	21	–	–
Kharchenko et al.	2016	1.63	1.29	–	313	–	–	–	–
Kharchenko et al.	2013	1.63	1.29	–	313	–	–	–	–
Dias et al.	2002	1.63	1.29	–	313	–	–	–	–

Visualization

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