Observability of atomic line features in strong magnetic fields

Details Observability of atomic line features in strong magnetic fields Observability of atomic line features in strong magnetic fields

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981xras.nasa..471w&link_type=abstract

In NASA. Goddard Space Flight Center X-ray Astronomy in the 1980's p 471-476 (SEE N82-26055 16-88)

Physics

Atomic Physics

Atomic Spectra, Magnetic Fields, Physical Properties, Atomic Physics, Electromagnetic Spectra, Lyman Spectra, X Ray Spectra

Scientific paper

The physical properties of atoms in superstrong magnetic fields, characteristic of neutron stars, and the possibility of detecting magnetically strongly shifted atomic lines in the spectra of magnetized X-ray pulsars are discussed. It is suggested that it is recommendable to look for magnetically strongly shifted Fe 26 Lyman lines in rotating neutron stars of not too high luminosity using spectrometers working in the energy range 10 - 20 keV, with sensitivities to minus 4 power photons per sq cm and second, and resolution E/delta E approx. 10-100.

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