A single exhaust model for backward emission in fast moving quasars

Details A single exhaust model for backward emission in fast moving quasars A single exhaust model for backward emission in fast moving quasars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983liaco..24..389s&link_type=abstract

IN: Quasars and gravitational lenses; Proceedings of the Twenty-fourth Liege International Astrophysical Colloquium, Cointe-Ougr

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Astronomical Spectroscopy, Quasars, Red Shift, Astrodynamics, Emission Spectra, Extragalactic Radio Sources, Intergalactic Media

Scientific paper

It is shown that the twin exhaust model of Blandford and Rees (1974) can be adapted to describe quasars moving rapidly through the intergalactic medium. The ram pressure of the intergalactic medium acts in such a way as to stop the forward jet and allow only the single jet in the backward direction. The model appears to satisfy all the gasdynamic and observational constraints imposed on it and offers an explanation for the paucity of radio loud quasars, the existence of a single jet in quasars, and why nebulosity is expected around redshift quasars.

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