Very-long-baseline radio interferometry

Details Very-long-baseline radio interferometry Very-long-baseline radio interferometry

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982prir........56m&link_type=abstract

Priroda, July 1982, p. 56-67. In Russian.

Astronomy and Astrophysics

Astronomy

High Resolution, Radio Sources (Astronomy), Very Long Base Interferometry, Bl Lacertae Objects, Galactic Nuclei, Interstellar Masers, Nebulae, Protoplanets, Quasars, Radio Galaxies, Radio Telescopes, Relativistic Electron Beams, Short Wave Radiation, Stellar Evolution

Scientific paper

The principle of operation of VLBI is explained. It is suggested that VLBI holds promise for the investigation of objects with active nuclei (i.e., quasars, radio galaxies, and BL Lac objects); the radio source Persei A, and the quasars 3C 345 and 3C 273 are discussed as examples of such objects. The future prospects of very-long-baseline interferometry are considered.

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