Cyclotron line formation in the magnetized atmospheres of compact stars – I. The transfer equations for polarized radiation-Reference-Cited by-同舟云学术

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Cyclotron line formation in the magnetized atmospheres of compact stars – I. The transfer equations for polarized radiation

Published:2016-03-28 Issue:2 Volume:459 Page:1847-1857
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Garasev M. A.,Derishev E. V.,Kocharovsky Vl. V.,Kocharovsky V. V.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/459/2/1847/8040658/stw711.pdf

Reference50 articles.

1. High-accuracy approximation of the complex probability function by Fourier expansion of exponential multiplier

2. Photon splitting and photon dispersion in a strong magnetic field

3. Cyclotron Line Features from Near‐critical Magnetic Fields: The Effect of Optical Depth and Plasma Geometry

4. Cyclotron‐Line Features from Near‐Critical Fields. II. On the Effect of Anisotropic Radiation Fields

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1. Spectral modification of magnetar flares by resonant cyclotron scattering;Monthly Notices of the Royal Astronomical Society;2020-08-08

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