The asymmetries in radio-source structures. 1: A comparison of two classical models

Details The asymmetries in radio-source structures. 1: A comparison of two classical models The asymmetries in radio-source structures. 1: A comparison of two classical models

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281...15r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 281, no. 1, p. 15-25

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Asymmetry, Doppler Effect, Extragalactic Radio Sources, Galactic Structure, Mathematical Models, Luminosity, Morphology, Power Series, Quasars

Scientific paper

A method is suggested for the mathematical description of the asymmetry occurring in the radio-source structures. The method is based on the transformation of the radio structure into 'itself' and may be used for all morphological types of structures. Two models of generation of the source asymmetry are investigated, namely Doppler effects and the flip-flop mechanism, with an assumption that the luminosity of the plasma volume depends on time as a power law S approximately tmu. The model with Doppler effects turns out to be more suitable than that with flip-flop mechanism.

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