Hostname: page-component-788cddb947-tr9hg Total loading time: 0 Render date: 2024-10-19T20:44:13.534Z Has data issue: false hasContentIssue false

The Cosmic Nozzle

Published online by Cambridge University Press:  25 May 2016

M.V. Konjukov*
Affiliation:
Astrospace Center of P. N. Lebedev Physics Institute of RAS Moscow Leninskii prospekt 53 Russia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The cosmic nozzle is a channel with flowing hot gas in a system containing the following components: stars, a hydrostatic gaseous corona and a cavity with hot gas in the central part of the system. In the quasi one-dimension approximation, the following solution of the cosmic nozzle problem about cosmic nozzle was obtained Here (ν,ω, T, σ) are the dimensionless density, hydro dynamical velocity, temperature and cross section of the channel (η0, ω0, T0 σ0 are these values at ζ = 1), φ(ζ), πg(ζ) are the gravitational potential and the pressure in the gaseous corona. For a polytropic state equation of the gas in the gaseous corona

Type
Radio Source Modelling and Emission Mechanisms
Copyright
Copyright © Kluwer 1996