A fast parallel code for calculating energies and oscillator strengths of many-electron atoms at neutron star magnetic field strengths in adiabatic approximation-Reference-Cited by-同舟云学术

A fast parallel code for calculating energies and oscillator strengths of many-electron atoms at neutron star magnetic field strengths in adiabatic approximation

Published:2009-02 Issue:2 Volume:180 Page:302-311
ISSN:0010-4655
Container-title:Computer Physics Communications
language:en
Short-container-title:Computer Physics Communications

Author:

Engel D.,Klews M.,Wunner G.

Publisher

Elsevier BV

Subject

General Physics and Astronomy,Hardware and Architecture

Reference61 articles.

1. 1RXS J214303.7+065419/RBS 1774: A new Isolated Neutron Star candidate

2. Discovery of Absorption Features in the X-Ray Spectrum of an Isolated Neutron Star

3. Pulse Phase Variations of the X‐Ray Spectral Features in the Radio‐quiet Neutron Star 1E 1207−5209

4. A broad absorption feature in the X-ray spectrum of the isolated neutron star RBS1223 (1RXS J130848.6+212708)

5. A phase-dependent absorption line in the spectrum of the X-ray pulsar RX J0720.4-3125

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