Rapid flux variations in compact radio sources: A shell model

Details Rapid flux variations in compact radio sources: A shell model Rapid flux variations in compact radio sources: A shell model

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cha%26a..11..100q&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 11, Issue 2, p. 100-104.

Astronomy and Astrophysics

Astrophysics

1

Radio Sources: Superluminal Phenomena

Scientific paper

In this paper, we discuss the flux variations of a shell whose expansion and bulk-motion are both at relativistic speeds. It is shown that superluminal flux variations can be produced even if the Lorentz factors of expansion and bulk-motion take moderate values (2-3), and that this kind of shell model suggested here could be significant for interpreting very rapid flux variations at centimeter wavelengths (time scale of 1-10 days) in some radio variable sources.

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