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De Falco, V., et al. (2017) The Transitional Millisecond Pulsar IGR J18245-2452 during Its 2013 Outburst at X-Rays and Soft Gamma-Rays. A&A, 603, A16.
https://doi.org/10.1051/0004-6361/201730600

has been cited by the following article:

• TITLE: Astrophysics: Macroobject Shell Model

  AUTHORS: Vladimir S. Netchitailo

  KEYWORDS: Hypersphere World-Universe Model, Medium of the World, Macroobject Shell Model, Dark Matter Particles, Gamma-Ray Bursts, Fast Radio Bursts, Multiwavelength Pulsars, Binary Millisecond Pulsars, Young Stellar Object Dippers, Starburst Galaxies, Gravitational Waves

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.3 No.4, October 31, 2017

  ABSTRACT: The model proposes that Nuclei of all macroobjects (Galaxy clusters, Galaxies, Star clusters, Extrasolar systems) are made up of Dark Matter Particles (DMP). These Nuclei are surrounded by Shells composed of both Dark and Baryonic matter. This model is used to explain various astrophysical phenomena: Multi-wavelength Pulsars; Binary Millisecond Pulsars; Gamma-Ray Bursts; Fast Radio Bursts; Young Stellar Object Dippers; Starburst Galaxies; Gravitational Waves. New types of Fermi Compact Stars made of DMP are introduced: Neutralino star, WIMP star, and DIRAC star. Gamma-Ray Pulsars are rotating Neutralino and WIMP stars. Merger of binary DIRAC stars can be a source of Gravitational waves.