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  2. Galaxy - Wikipedia

    en.wikipedia.org/wiki/Galaxy

    Types of galaxies according to the Hubble classification scheme : an E indicates a type of elliptical galaxy; an S is a spiral; and SB is a barred spiral galaxy. Galaxies come in three main types: ellipticals, spirals, and irregulars. A slightly more extensive description of galaxy types based on their appearance is given by the Hubble sequence.

  3. List of galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_galaxies

    In the 1980s, the Lyons Groups of Galaxies listed 485 galaxy groups with 3,933 member galaxies. Galaxy Zoo is a project aiming at a more comprehensive list: launched in July 2007, it has classified over one million galaxy images from The Sloan Digital Sky Survey, The Hubble Space Telescope and the Cosmic Assembly Near-Infrared Deep ...

  4. Stingray Music - Wikipedia

    en.wikipedia.org/wiki/Stingray_Music

    Original logo of Galaxie from 1997 to 2000. From 2000 to 2003, the orange circle was removed. The service's beginnings in Canada started in December 1995, when the Canadian Broadcasting Corporation was granted approval from the Canadian Radio-television and Telecommunications Commission (CRTC) to launch a national pay audio service named Galaxie consisting of 30 channels in both English and ...

  5. Radio galaxy - Wikipedia

    en.wikipedia.org/wiki/Radio_galaxy

    The problem with this method is that hosts of active galaxies may not be typical of galaxies at their redshift. Similarly, radio galaxies have in the past been used to find distant X-ray emitting clusters, but unbiased selection methods are now preferred. The most distant radio galaxy currently known is TGSS J1530+1049, at a redshift of 5.72. [23]

  6. Satellite galaxy - Wikipedia

    en.wikipedia.org/wiki/Satellite_galaxy

    Remnants of a minor merger can be observed in the form of a stellar stream falling onto the galaxy NGC 5907. Throughout their lifespan, satellite galaxies orbiting in the dark matter halo experience dynamical friction and consequently descend deeper into the gravitational potential of their host as a result of orbital decay.

  7. Free streaming - Wikipedia

    en.wikipedia.org/wiki/Free_streaming

    An often used definition for the surface of a star is based on the path that photons take. Inside a star, photons travel by random walk , constantly interacting with matter, and the surface of the star is defined as the point at which photons encounter little resistance from the matter in the stellar atmosphere , or in other words, when photons ...

  8. Local Group - Wikipedia

    en.wikipedia.org/wiki/Local_Group

    The term "The Local Group" was introduced by Edwin Hubble in Chapter VI of his 1936 book The Realm of the Nebulae. [11] There, he described it as "a typical small group of nebulae which is isolated in the general field" and delineated, by decreasing luminosity, its members to be M31, Milky Way, M33, Large Magellanic Cloud, Small Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC 1613 and ...

  9. Galactic astronomy - Wikipedia

    en.wikipedia.org/wiki/Galactic_astronomy

    This is in contrast to extragalactic astronomy, which is the study of everything outside our galaxy, including all other galaxies. Galactic astronomy should not be confused with galaxy formation and evolution , which is the general study of galaxies , their formation, structure, components, dynamics, interactions, and the range of forms they take.