Markarian 50

(MWSC 3712; Mrk 50)

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0.83 UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad) 18.3 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.81 Well-studied
  • Cdup 1.0 Unique

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 well-studied in the literature.

(*): The parallax distance estimate (~3.11 kpc) differs significantly from the median photometric distance (~2.36 kpc).

Palma et al. (2025)
Part of multiple system G198, along with HSC_880, CWNU_2651 and CWNU_2203.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Data

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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 –
Dias et al. 2018 – – – -3.99 -2.51 –
Loktin & Popova 2017 348.78 60.436 – -0.464 -1.643 -81.0
Sampedro et al. 2017 348.825 60.467 -2.95 0.91 – –
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
Bukowiecki et al. 2011 348.792 60.438 – – – –
Kharchenko et al. 2007 348.82 60.47 – 0.02 – –
Ahumada & Lapasset 2007 348.825 60.467 – – – –
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 – – – –
Lynga 1987 348.825 60.494 – – – -81.0

💡 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] Bfrac BSS
UCC 99999– 2.36 2.47 1.14 13 -0.077 309 – 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 2.56 – 12 – – – 0
Dias et al. 2021 2.68 2.24 – 13 -0.054 – – –
Cantat-Gaudin et al. 2020 3.21 2.35 – 11 – – – –
Kounkel et al. 2020 2.89 2.25 – 21 – – – –
Cantat-Gaudin & Anders 2020 2.84 – – – – – – –
Cantat-Gaudin et al. 2018 2.84 – – – – – – –
Loktin & Popova 2017 2.11 2.47 – 15 – – – –
Kharchenko et al. 2016 2.30 2.56 – 13 – – – –
Kharchenko et al. 2013 2.30 2.56 – 13 – – – –
Bukowiecki et al. 2012 – – – – – 309 – –
Kharchenko et al. 2012 2.30 2.56 – 13 – – – –
Bukowiecki et al. 2011 1.70(1) 1.64 – 126 – – – –
Ahumada & Lapasset 2007 – 2.56 – 13 – – – 0
van den Bergh 2006 2.11 2.56 – 13 – – – –
Dias et al. 2002 2.11 2.56 – 12 – – – –
Dambis 1999 1.78 2.28 – 13 – – – –
Lynga 1987 2.25 2.62 – 10 – – – –

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

Visualization

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