3C 279 (also known as 4C–05.55, NRAO 413, and PKS 1253–05) is an optically violent variable quasar (OVV), which is known in the astronomical community...
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Event Horizon Telescope (section 3C 279)
the first 20 microarcsecond resolution images of the archetypal blazar 3C 279 it observed in April 2017. These images, generated from observations over...
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appearance to BL Lac objects but generally have stronger broad emission lines. 3C 279 S5 0014+81 "APEX takes part in sharpest observation ever". ESO Press Release...
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why, 16 March 1991 The superluminal radio source in the gamma-ray blazar 3C 279 Porcas, R. W (1981). "Superluminal quasar 3C179 with double radio lobes"...
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; Roberts, D. H. (1998). "Electron-positron Jets Associated with Quasar 3C 279" (PDF). Nature. 395 (6701): 457. Bibcode:1998Natur.395..457W. doi:10.1038/26675...
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quasar 3C 9 is cited by Kardashev as early as 1971. The study of the quasar 3C 273 shows that it has a solid structure. Other quasars (3C 279, 3C 345, 3C 84)...
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doi:10.1103/PhysRev.126.1818. "Electron-positron Jets Associated with Quasar 3C 279" (PDF). "Vast Cloud of Antimatter Traced to Binary Stars". NASA. https://www...
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1086/317769. S2CID 17274015. Electron–positron Jets Associated with Quasar 3C 279 Naeye, R.; Gutro, R. (2008-01-09). "Vast Cloud of Antimatter Traced to Binary...
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and Australia. The change in the source visibility that they measured for 3C 279, combined with changes in total flux density, indicated that a component...
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45, ON 231, 3C 273, 3C 279, PKS 1510−08, DA 406, 4C 38.41, 3C 345, Markarian 501, 4C 51.37, 3C 371, PKS 2155−304, BL Lacertae, CTA 102, 3C 454.3 and 1ES...
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