Open AccessJournal Article
Rotating neutron star models with a magnetic field.
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This article is published in Astronomy and Astrophysics.The article was published on 1995-09-01 and is currently open access. It has received 181 citations till now. The article focuses on the topics: Neutron star & Theory of relativity.read more
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Book ChapterDOI
Multi-Fluid Models of Astrophysical Plasma
TL;DR: The multi-fluid models of plasma in electric and magnetic fields allow us to consider important properties of astrophysical plasma, in particular the Langmuir and electromagnetic waves, as well as many other interesting effects and applications as discussed by the authors.
Journal ArticleDOI
Estimating magnetar radii with an empirical meta-model
TL;DR: In this article, the effect of strong magnetic fields on spinodal instabilities of neutron star matter and the associated crust-core properties was investigated using a meta-modeling technique that allows exploring the model dependence of density functional theory equation of state calculations.
Book ChapterDOI
Single-Fluid Models for Astrophysical Plasma
Abstract: Single-fluid models are the simplest but sufficient approximation to describe many large-scale low-frequency phenomena in astrophysical plasma: regular and turbulent dynamo, plasma motions driven by strong magnetic fields, accretion disks, and relativistic jets.
Book ChapterDOI
Macroscopic Description of Astrophysical Plasma
TL;DR: In this paper, the authors treat individual kinds of particles as continuous media, mutually penetrating charged gases which interact between themselves and with an electromagnetic field, and give us the multi-fluid model which is useful to consider many properties of astrophysical plasmas, for example, the solar wind.
Book ChapterDOI
Particle Acceleration by Shock Waves
TL;DR: In this paper, shocks are widely recognized as a key to understanding high-energy particle acceleration in a variety of astrophysical environments, and they have been used to accelerate cosmic rays.