Markarian 50

(MWSC 3712; Mrk 50)

0.90 UTI

0.52

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 54

Stellar density (N₅₀/rad) 18.3 [N/pc²]

C3 classification AA

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Markarian 50 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Markarian 50 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	99999–	348.809	60.448	0.322	-3.414	-2.628	–
Almeida et al.	2025	348.812	60.451	–	–	–	–
Hunt & Reffert	2024	348.809	60.44	0.328	-3.398	-2.648	–
Celli et al.	2024	348.806	60.448	–	–	–	–
Cavallo et al.	2024	348.811	60.448	0.326	–	–	–
Hunt & Reffert	2023	348.809	60.44	0.328	-3.398	-2.648	–
Just et al.	2023	348.806	60.43	–	–	–	–
Jaehnig et al.	2021	348.806	60.439	0.346	-3.438	-2.562	–
Rain et al.	2021	348.806	60.448	0.323	-3.465	-2.56	–
Dias et al.	2021	348.812	60.451	0.317	-3.495	-2.568	–
Cantat-Gaudin et al.	2020	348.806	60.448	0.323	-3.465	-2.56	–
Cantat-Gaudin & Anders	2020	348.806	60.448	0.323	-3.465	-2.56	–
Cantat-Gaudin et al.	2018	348.806	60.448	0.323	-3.465	-2.56	–
Loktin & Popova	2017	348.78	60.436	–	-0.464	-1.643	-81.0
Kharchenko et al.	2016	348.806	60.43	–	–	–	–
Kharchenko et al.	2013	348.813	60.434	–	-0.31	-1.54	-81.0
Kharchenko et al.	2012	348.813	60.434	–	-0.31	-1.54	-81.0
Kharchenko et al.	2007	348.82	60.47	–	0.02	–	–
van den Bergh	2006	348.809	60.448	–	–	–	–
Dias et al.	2002	348.825	60.467	–	-0.96	-6.43	–
Dambis	1999	348.807	60.45	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	2.52	2.42	1.14	13	-0.077	319	–	0.0
Almeida et al.	2025	2.68	2.24	–	13	–	331	–	–
Hunt & Reffert	2024	–	–	–	–	–	583⁽¹⁾	–	–
Celli et al.	2024	–	–	–	12	–	307	–	–
Cavallo et al.	2024	2.36	2.24	–	25	-0.100	–	–	–
Hunt & Reffert	2023	2.78	2.41	1.14	12	–	–	–	–
Just et al.	2023	–	–	–	13	–	78	–	–
Jaehnig et al.	2021	2.86⁽¹⁾	–	–	–	–	–	–	–
Rain et al.	2021	2.84	2.51	–	12	–	–	–	0
Dias et al.	2021	2.68	2.24	–	13	-0.054	–	–	–
Cantat-Gaudin et al.	2020	3.21	2.35	–	11	–	–	–	–
Cantat-Gaudin & Anders	2020	2.84	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.84	–	–	–	–	–	–	–
Loktin & Popova	2017	2.11	2.42	–	15	–	–	–	–
Kharchenko et al.	2016	2.30	2.51	–	13	–	–	–	–
Kharchenko et al.	2013	2.30	2.51	–	13	–	–	–	–
Kharchenko et al.	2012	2.30	2.51	–	13	–	–	–	–
van den Bergh	2006	2.11	2.51	–	13	–	–	–	–
Dias et al.	2002	2.11	2.51	–	12	–	–	–	–
Dambis	1999	1.78	2.24	–	13	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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