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Theory of Disk Accretion onto Magnetic Stars

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arxiv 1402.1903 v1 pith:OCIO7ANH submitted 2014-02-09 astro-ph.SR astro-ph.HE

Dong Lai This is my paper
classification astro-ph.SRastro-ph.HE
keywords starsmagneticaccretingaccretiondiskneutronontosome
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Disk accretion onto magnetic stars occurs in a variety of systems, including accreting neutron stars (with both high and low magnetic fields), white dwarfs, and protostars. We review some of the key physical processes in magnetosphere-disk interaction, highlighting the theoretical uncertainties. We also discuss some applications to the observations of accreting neutron stars and protostellar systems, as well as possible connections to protoplanetary disks and exoplanets.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Gamma-ray lines, electron-positron annihilation, and possible radio emission in X-ray pulsars

    astro-ph.HE 2025-09 conditional novelty 6.0 of 10

    Accreting X-ray pulsars are predicted to produce detectable gamma-ray lines at 2.2-67.5 MeV plus a 511 keV annihilation line, with observability limited by magnetospheric absorption and radiative deceleration.

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