Quasars at 25
- 10 October 1986
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 234 (4773) , 155-161
- https://doi.org/10.1126/science.234.4773.155
Abstract
In the quarter century since the first optical identification of a "radio star" (3C 48), astronomers have come to general agreement that the underlying quasar energy source is accretion onto a massive black hole. There is much less agreement on the detailed physics of the processes by which this energy is converted to the forms observed, but this has not prevented the objects from serving as valuable probes of the universe at distant times and places.Keywords
This publication has 100 references indexed in Scilit:
- Test of the gravitational lens hypothesis for the quasar pair 1146+111B,CNature, 1986
- The central engine of quasars and active galactic nuclei Hadronic interactions of shock-accelerated relativistic protonsThe Astrophysical Journal, 1986
- An apparent gravitational lens with an image separation of 2.6 arc minNature, 1986
- H 0323 + 022 - A new BL Lacertae object with extremely rapid variabilityThe Astrophysical Journal, 1986
- Radio emission from the jet and lobe of 3C273Nature, 1985
- Pavo XD-10, an X-ray QSO with extended optical structureNature, 1985
- Nine new quasi-stellar objects with broad absorption linesThe Astrophysical Journal, 1984
- The Small-Scale Structure of Radio Galaxies and Quasi-Stellar Sources at 3.8 CentimetersThe Astrophysical Journal, 1971
- Quasars Revisited: Rapid Time Variations Observed Via Very-Long-Baseline InterferometryScience, 1971
- Investigation of the Radio Source 3C 273 By The Method of Lunar OccultationsNature, 1963