Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-12T09:51:48.247Z Has data issue: false hasContentIssue false

Particle Acceleration and Radiation in Magnetospheres of Collapsing Stars

Published online by Cambridge University Press:  25 May 2016

V. Kryvdyk*
Affiliation:
Department of Astronomy, Kiev University, Glushkova 6, UKR-252022, Kiev, Ukraine

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.

Particle dynamics and nonthermal emission therefrom in the magnetospheres of collapsing stars with initial dipole magnetic fields and a certain initial energy distribution of charged particles (power-law, relativistic Maxwell, and Boltzmann distributions) are considered. The radiation fluxes are calculated for various collapsing stars with initial dipole magnetic fields and an initial power-law particle energy distribution in the magnetosphere. The effects can be observed by means of modern instruments.

Type
Part II: Posters
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Angel, J. R. P. 1978, ARAA, 16, 487.CrossRefGoogle Scholar
Ginzburg, V. L., & Syrovatskii, S. I. 1963, Origin of cosmic rays (Moscow: Izdatel'stvo Akademiji Nauk USSR).Google Scholar
Güdel, M., & Benz, A. O. 1996, in ASP Conf. Ser. Vol. 93, Radio Emission from the Stars and the Sun, eds. Taylor, A. R. & Paredes, J. M. (Barcelona: ASP), 303.Google Scholar
Kryvdyk, V. 1999, MNRAS, 309, 593.CrossRefGoogle Scholar
Shapiro, S. L., & Teukolsky, S. A. 1985, Black Holes, White Dwarfs, and Neutron Stars (Moscow: Mir).Google Scholar
Utana, G., Trigilio, C., & Catalano, S. 1998, AAP, 329, 1010.Google Scholar