Hostname: page-component-669899f699-7tmb6 Total loading time: 0 Render date: 2025-04-26T08:34:00.763Z Has data issue: false hasContentIssue false
  • English
  • Français

On a Possible Influence of Magnetic Fields on the Structure of a Disk Formed During Accretion of Plasma in Binary Systems

Published online by Cambridge University Press:  07 February 2017

L. A. Pustilnik  and
V. F. Shvartsman
L. A. Pustilnik
Affiliation:
Special Astrophysical Observatory, U.S.S.R. Academy of Sciences, St. Zelenchukskaya, Stavropolskij Kraj 357140, U.S.S.R.
V. F. Shvartsman
Affiliation:
Special Astrophysical Observatory, U.S.S.R. Academy of Sciences, St. Zelenchukskaya, Stavropolskij Kraj 357140, U.S.S.R.

Abstract

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.

During accretion of plasma in binary systems containing compact objects magnetic fields are most likely to become arranged quickly, grow and fully determine the disk structure. The disk divides into separate dense clots, and a corona appears over the equatorial plane of the system. In the corona magnetic lines of force reconnect and beams of relativistic particles are generated.

Type
Part III: Accretion of Matter and X-Ray Sources
Information
Symposium - International Astronomical Union , Volume 64: Gravitational Radiation and Gravitational Collapse , 1974 , pp. 213
Copyright
Copyright © Reidel 1974 

References

Pustilnik, L. A. and Shvartsman, V. F.: 1973, Commun. SAO U.S.S.R. AS, in press.Google Scholar