Quasars - Quasar, List of Quasars, He0450-2958, So Tan Argument, Oj 287, 3c 48, Multiply Imaged Quasar, Quasar J1819+3845 (Paperback)

Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Pages: 116. Not illustrated. Chapters: Quasar, List of Quasars, He0450-2958, So tan Argument, Oj 287, 3c 48, Multiply Imaged Quasar, Quasar J1819+3845, Laser Star Model of Quasars, Q0906+6930, Cta-102, Qso J0842+1835, Apm 08279+5255, Qso B0307+169, Qso B0220+427, Qso B1637+826, Qso B0316+413, 3c 286, 3c 35, Qso B0104+321, Qso B2243+394, Qso B2121+248, Qso B0917+458, Qso B1522+546, Qso B0958+290, Qso B1203+645, Qso B0936+361, Qso B1409+524, Qso B1419+419, Qso B0702+749, 3c 212, Qso B1441+5214, Lbqs 1429-008, 3c 9, Qso B0038+328, 2mass J07491255+5552336, 3c 191, Ovv Quasar, Blandford-Znajek Process. Excerpt: This is a list of quasars. Proper naming of quasars are by Catalogue Entry, Qxxxx yy using B1950 coordinates, or QSO Jxxxx yyyy using J2000 coordinates. They may also use the prefix QSR. This is a list of quasars, with a common name, instead of a designation from a survey, catalogue or list. There are currently no quasars that are visible to the naked eye. This is a list of quasars, that as a result of gravitational lensing, appears as multiple images on Earth. This is a list of double quasars, triple quasars, and the like, where quasars are close together in line-of-sight, but not physically related. This is a lise of binary quasars, trinary quasars, and the like, where quasars are physically close to each other. This is a list of quasars with jets that appear to be superluminal due to relativistic effects and line-of-sight orientation. Such quasars are sometimes referred to as superluminal quasars. It should be noted that quasars that have a recessional velocity greater than the speed of light (c) are very common. Any quasar with z>1 is going away from us in excess of c. Early attempts to explain superlumic quasars resulted in convoluted explanations with a limit of z=2.326, or in the extreme z