Ruprecht 141

(MWSC 2935; OCL 60)

0.35 UTI

0.0

C_N

0.1

C_dens

0.38

C_C3

0.65

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 13

Radius (P>50% members) 5.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.38 Low quality
C_lit 0.65 Moderately studied
C_dup 1.0 Unique

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

Overview

ℹ️

Ruprecht 141 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as an extremely massive, very young cluster (see Parameters). It is moderately studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Extremely massive Very young

Data

🔍 Search references for Ruprecht 141 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	277.817	-12.333	0.325	-1.469	-4.255	20.693
Just et al.	2023	277.821	-12.327	–	–	–	–
Bica et al.	2019	277.845	-12.298	–	–	–	–
Kharchenko et al.	2016	277.821	-12.327	–	–	–	–
Dias et al.	2014	277.825	-12.317	–	-1.13	-0.76	–
Kharchenko et al.	2013	277.828	-12.326	–	-1.79	-1.27	30.7
Gozha et al.	2012	277.825	-12.317	–	–	–	–
Piskunov et al.	2008	277.822	-12.32	–	–	–	–
Kharchenko et al.	2007	277.83	-12.32	–	0.11	–	30.7
Kharchenko et al.	2005	277.83	-12.32	–	0.57	-2.68	30.7
Kharchenko et al.	2003	277.83	-12.3	–	1.37	-4.67	–
Dias et al.	2002	277.825	-12.317	–	-1.13	-0.76	30.7

💡 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	–	–	–	4	–	701	–	–
Kharchenko et al.	2016	3.38	2.94	–	4	–	–	–	–
Kharchenko et al.	2013	3.38	2.94	–	4	–	–	–	–
Gozha et al.	2012	1.43	–	–	30	–	22387	–	–
Piskunov et al.	2008	5.50	1.77	–	8	–	–	–	–
Kharchenko et al.	2005	5.50	1.77	–	8	–	–	–	–
Kharchenko et al.	2003	1.43	0.31	–	–	–	–	–	–
Dias et al.	2002	1.80	1.40	–	30	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gulliver 41	8.0	277.72	-12.43	0.18	-1.7	-4.77	58.1	0.57

💡 Note: The % column shows the percentage of members that Ruprecht 141 shares with each listed object.

Visualization

ℹ️