Radio properties and arm classification in spiral galaxies

Details Radio properties and arm classification in spiral galaxies Radio properties and arm classification in spiral galaxies

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..259g&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

Radio Galaxies, Spiral Galaxies, Classifications, Continuous Spectra, Density Wave Model

Scientific paper

An investigation of the radio continuum properties of the spiral galaxies which have been classified in the Elmegreen and Elmegreen (1987) arm morphology system reveals no difference in the radio continuum emission (per light unit) for flocculent and grand design spirals. Nor is the X-ray emission (per light unit) of the two classes of spirals different. Furthermore, it is found that flocculent galaxies are more frequently encountered in samples of interacting and binary galaxies than among relatively isolated objects.

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