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  • Astrophysics - Wikipedia
    Theorists in astrophysics endeavor to create theoretical models and figure out the observational consequences of those models This helps allow observers to look for data that can refute a model or help in choosing between several alternate or conflicting models
  • Category:Astrophysics - Wikipedia
    Astrophysics is the branch of astronomy that deals with the physics of the universe, including the physical properties (luminosity, density, temperature, chemical composition) of astronomical objects such as stars, galaxies, and the interstellar medium, as well as their interactions
  • Astroparticle physics - Wikipedia
    Astroparticle physics, also called particle astrophysics, is a branch of particle physics that studies elementary particles of astrophysical origin and their relation to astrophysics and cosmology
  • Nuclear astrophysics - Wikipedia
    Nuclear astrophysics studies the origin of the chemical elements and isotopes, and the role of nuclear energy generation, in cosmic sources such as stars, supernovae, novae, and violent binary-star interactions
  • Accretion (astrophysics) - Wikipedia
    In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, into an accretion disk [1][2] Most astronomical objects, such as galaxies, stars, and planets, are formed by accretion processes
  • Astrophysics - Simple English Wikipedia, the free encyclopedia
    Astrophysics is the study of how stars, planets, and other things in the Universe work, and how we can learn about them Astrophysicists use physics and chemistry to explain what astronomers find and see
  • Astronomy Astrophysics - Wikipedia
    Astronomy Astrophysics (A A)[1] is a monthly peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics
  • Astronomical spectroscopy - Wikipedia
    Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, ultraviolet, X-ray, infrared and radio waves that radiate from stars and other celestial objects


















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