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  2. Category:Black-and-white photographs - Wikipedia

    en.wikipedia.org/wiki/Category:Black-and-white...

    Specific black-and-white photographs. It should not contain the images (files) themselves, nor should it contain free- or fair-use images which do not have associated articles. See also Category:Color photographs

  3. Centaurus A - Wikipedia

    en.wikipedia.org/wiki/Centaurus_A

    The galaxy's strange morphology is generally recognized as the result of a merger between two smaller galaxies. [34] Zoom movie of the galaxy Centaurus A, showing different aspects of the galaxy in several wavelengths. Schematic diagram of the components of the Centaurus A galaxy. The bulge of this galaxy is composed mainly of evolved red stars ...

  4. NGC 4622 - Wikipedia

    en.wikipedia.org/wiki/NGC_4622

    The spiral galaxy NGC 4622 lies approximately 111 million light-years away from Earth in the constellation Centaurus. NGC 4622 is an example of a galaxy with leading spiral arms . [ 2 ] Each spiral arm winds away from the center of the galaxy and ends at an outermost tip that "points" in a certain direction (away from the arm).

  5. TON 618 - Wikipedia

    en.wikipedia.org/wiki/TON_618

    Size comparison of the event horizons of the black holes of TON 618 and Phoenix A.The orbit of Neptune (white oval) is included for comparison. As a quasar, TON 618 is believed to be the active galactic nucleus at the center of a galaxy, the engine of which is a supermassive black hole feeding on intensely hot gas and matter in an accretion disc.

  6. NGC 2835 - Wikipedia

    en.wikipedia.org/wiki/NGC_2835

    The star formation rate in NGC 2835 is 1.3 M ☉ per year and the total stellar mass of the galaxy is 10 10 M ☉. [7] In the centre of NGC 2835 lies a supermassive black hole whose mass is estimated to be 3-10 million (10 6.72±0.3) M ☉, based on the spiral arm pitch angle. [8] NGC 2835 is the foremost galaxy in a small group of galaxies ...

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  8. Cygnus A - Wikipedia

    en.wikipedia.org/wiki/Cygnus_A

    The supermassive black hole at the core has a mass of (2.5 ± 0.7) × 10 9 M ☉. [3] Images of the galaxy in the radio portion of the electromagnetic spectrum show two jets protruding in opposite directions from the galaxy's center. These jets extend many times the width of the portion of the host galaxy which emits radiation at visible ...

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