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Brands, S.A., de Koter, A., Bestenlehner, J., Crowther, P., Sundqvist, J., Puls, J., et al. (2022) The R136 Star Cluster Dissected with Hubble Space Telescope/STIS. III. The Most Massive Stars and Their Clumped Winds. Astronomy & Astrophysics, Forthcoming Article. arXiv:2202.11080.
https://doi.org/10.1051/0004-6361/202142742

has been cited by the following article:

• TITLE: Center of Milky Way Galaxy

  AUTHORS: Vladimir S. Netchitailo

  KEYWORDS: World-Universe Model, Center of Milky Way Galaxy, Supermassive Compact Object, Event Horizon Telescope, Sagittarius A*, Multi-Component Dark Matter, Macroobjects Shell Model, Angular Momentum Problem

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.8 No.3, July 21, 2022

  ABSTRACT: In 2013, World-Universe Model (WUM) made one of the most important predictions: “Macroobjects of the World have cores made up of the discussed DM (Dark Matter) particles. Other particles, including DM and baryonic matter, form shells surrounding the cores” [1]. Prof. R. Genzel and A. Ghez confirmed this prediction: “The Discovery of a Supermassive Compact Object at the Centre of Our Galaxy” (Nobel Prize in Physics 2020). On May 12, 2022, astronomers, using the Event Horizon Telescope, released the first image of the accretion disk around the Sagittarius A* (Sgr A*) produced using a worldwide network of radio observatories made in April 2017. These observations were obtained by a global array of millimeter wavelength telescopes and analyzed by an international research team that now numbers over 300 people, which claimed that Sgr A* is a Supermassive Black Hole (SBH). In the present paper, we analyze these results in frames of WUM. Based on the totality of all accumulated experimental results for the Center of the Milky Way Galaxy we conclude that Sgr A* is the DM Core of our Galaxy.