Evolutionary effects of a supermassive body on a large surrounding cloud

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrophysics, Celestial Bodies, Rotating Bodies, Galactic Nuclei, Magnetic Dipoles, Magnetic Flux, Quasars, Radiation Sources, Radiation Spectra, Relativistic Particles, Supermassive Stars

Scientific paper

The possibility that spinning massive bodies with high surface magnetic field are the main energy sources in some extragalactic system (QSOs, Seyfert nuclei, etc) has led the authors to study the dynamical evolution of a spherically symmetric cloud containing a spinar in its centre. The spinar is assumed to lose energy through the magnetic dipole mechanism. This energy, transformed in magnetic field and particles energy, produces a pressure force pushing outwards the surrounding matter. The process leads to the formation of a cavity around the spinar, filled with relativistic electrons and magnetic field. The dynamical evolution of the cavity and the spectral evolution of its radiation is studied.

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