FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2896501904> ?p ?o ?g. }

• W2896501904 endingPage "46" @default.
• W2896501904 startingPage "1" @default.
• W2896501904 abstract "The inner regions of active galaxies host the most extreme and energetic phenomena in the universe including, relativistic jets, supermassive black hole binaries, and recoiling supermassive black holes. However, many of these sources cannot be resolved with direct observations. I review how strong gravitational lensing can be used to elucidate the structures of these sources from radio frequencies up to very high energy gamma rays. The deep gravitational potentials surrounding galaxies act as natural gravitational lenses. These gravitational lenses split background sources into multiple images, each with a gravitationally-induced time delay. These time delays and positions of lensed images depend on the source location, and thus, can be used to infer the spatial origins of the emission. For example, using gravitationally-induced time delays improves angular resolution of modern gamma-ray instruments by six orders of magnitude, and provides evidence that gamma-ray outbursts can be produced at even thousands of light years from a supermassive black hole, and that the compact radio emission does not always trace the position of the supermassive black hole. These findings provide unique physical information about the central structure of active galaxies, force us to revise our models of operating particle acceleration mechanisms, and challenge our assumptions about the origin of compact radio emission. Future surveys, including LSST, SKA, and Euclid, will provide observations for hundreds of thousands of gravitationally lensed sources, which will allow us to apply strong gravitational lensing to study the multi-wavelength structure for large ensembles of sources. This large ensemble of gravitationally lensed active galaxies will allow us to elucidate the physical origins of multi-wavelength emissions, their connections to supermassive black holes, and their cosmic evolution." @default.
• W2896501904 created "2018-10-26" @default.
• W2896501904 creator A5055616996 @default.
• W2896501904 date "2018-12-01" @default.
• W2896501904 modified "2023-10-17" @default.
• W2896501904 title "Gravitational lenses as high-resolution telescopes" @default.
• W2896501904 cites W1024987255 @default.
• W2896501904 cites W1495510671 @default.
• W2896501904 cites W1497346607 @default.
• W2896501904 cites W1501370474 @default.
• W2896501904 cites W1551745221 @default.
• W2896501904 cites W1871221100 @default.
• W2896501904 cites W1878238285 @default.
• W2896501904 cites W1891583834 @default.
• W2896501904 cites W190758278 @default.
• W2896501904 cites W1927416654 @default.
• W2896501904 cites W1964440768 @default.
• W2896501904 cites W1964927878 @default.
• W2896501904 cites W1965431757 @default.
• W2896501904 cites W1971687220 @default.
• W2896501904 cites W1972402856 @default.
• W2896501904 cites W1973497701 @default.
• W2896501904 cites W1974526556 @default.
• W2896501904 cites W1974545003 @default.
• W2896501904 cites W1974913150 @default.
• W2896501904 cites W1975480893 @default.
• W2896501904 cites W1976447431 @default.
• W2896501904 cites W1978498913 @default.
• W2896501904 cites W1978514484 @default.
• W2896501904 cites W1979115990 @default.
• W2896501904 cites W1979498879 @default.
• W2896501904 cites W1981138880 @default.
• W2896501904 cites W1982663784 @default.
• W2896501904 cites W1985293929 @default.
• W2896501904 cites W1986316936 @default.
• W2896501904 cites W1988597271 @default.
• W2896501904 cites W1989263666 @default.
• W2896501904 cites W1989266201 @default.
• W2896501904 cites W1989941187 @default.
• W2896501904 cites W1992842520 @default.
• W2896501904 cites W1994576009 @default.
• W2896501904 cites W1994761351 @default.
• W2896501904 cites W1995061453 @default.
• W2896501904 cites W1995568970 @default.
• W2896501904 cites W1996102612 @default.
• W2896501904 cites W1996742276 @default.
• W2896501904 cites W1997374481 @default.
• W2896501904 cites W2001981887 @default.
• W2896501904 cites W2008725538 @default.
• W2896501904 cites W2013171719 @default.
• W2896501904 cites W2013198578 @default.
• W2896501904 cites W2013352950 @default.
• W2896501904 cites W2017881043 @default.
• W2896501904 cites W2018140110 @default.
• W2896501904 cites W2019185840 @default.
• W2896501904 cites W2020174624 @default.
• W2896501904 cites W2021007172 @default.
• W2896501904 cites W2022902136 @default.
• W2896501904 cites W2023347320 @default.
• W2896501904 cites W2024769643 @default.
• W2896501904 cites W2026926262 @default.
• W2896501904 cites W2027853886 @default.
• W2896501904 cites W2028382975 @default.
• W2896501904 cites W2028998331 @default.
• W2896501904 cites W2031254971 @default.
• W2896501904 cites W2032876862 @default.
• W2896501904 cites W2033187319 @default.
• W2896501904 cites W2033220168 @default.
• W2896501904 cites W2033802241 @default.
• W2896501904 cites W2034169934 @default.
• W2896501904 cites W2036247675 @default.
• W2896501904 cites W2036377689 @default.
• W2896501904 cites W2036385708 @default.
• W2896501904 cites W2036920580 @default.
• W2896501904 cites W2037909731 @default.
• W2896501904 cites W2038367995 @default.
• W2896501904 cites W2038877798 @default.
• W2896501904 cites W2040619705 @default.
• W2896501904 cites W2041043641 @default.
• W2896501904 cites W2042039095 @default.
• W2896501904 cites W2043345349 @default.
• W2896501904 cites W2044714607 @default.
• W2896501904 cites W2044991242 @default.
• W2896501904 cites W2045399005 @default.
• W2896501904 cites W2045551905 @default.
• W2896501904 cites W2047085668 @default.
• W2896501904 cites W2047427095 @default.
• W2896501904 cites W2049067536 @default.
• W2896501904 cites W2049166557 @default.
• W2896501904 cites W2050399495 @default.
• W2896501904 cites W2052514468 @default.
• W2896501904 cites W2053222792 @default.
• W2896501904 cites W2053955485 @default.
• W2896501904 cites W2056212783 @default.
• W2896501904 cites W2056713841 @default.
• W2896501904 cites W2057504741 @default.
• W2896501904 cites W2057862339 @default.
• W2896501904 cites W2058663274 @default.

• next