Probing the Cores of Radio Jets through Interstellar Scintillation

Details Probing the Cores of Radio Jets through Interstellar Scintillation Probing the Cores of Radio Jets through Interstellar Scintillation

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007rmxac..27..129r&link_type=abstract

Triggering Relativistic Jets (Eds. William H. Lee & Enrico Ramírez-Ruiz) Revista Mexicana de Astronomía y Astrofísica (Serie de

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Quasars: Ism

Scientific paper

Interstellar Scintillation (ISS) has been established as the cause of the random variations in compact radio radio sources on times of a day or less. This interpretation provides quantitative information on the structure of the inner regions of the Radio-Emitting Jets on scales down to 10 μarcsec, once the distance to the scattering region is known. In turn these imply Doppler factors 5-75, which are on the same order as derived from VLB interferometry.

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