Relationship between the spectra of scintillating radio sources and the morphological type of active galaxies

Details Relationship between the spectra of scintillating radio sources and the morphological type of active galaxies Relationship between the spectra of scintillating radio sources and the morphological type of active galaxies

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..268a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, April 1987, p. 268-274. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Active Galaxies, Elliptical Galaxies, Radio Galaxies, Radio Sources (Astronomy), Radio Spectra, Scintillation, Spiral Galaxies, Galactic Nuclei, Galactic Structure, Interstellar Magnetic Fields, Point Sources, Quasars, Spectrum Analysis

Scientific paper

Interplanetary scintillation observations of active galaxies at a frequency of 102 MHz are analyzed. It is shown that scintillating components with flat or inverted spectra are mainly giant elliptical galaxies, while components with steep spectra are mainly spiral galaxies. Physical conditions in the nuclei of these galaxies are considered.

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