Model for 1.24 S X-ray pulses in HER X-1

Details Model for 1.24 S X-ray pulses in HER X-1 Model for 1.24 S X-ray pulses in HER X-1

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..250f&link_type=abstract

Nature, vol. 253, Jan. 24, 1975, p. 250, 251.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Magnetic Stars, Neutron Stars, Pulsed Radiation, X Ray Stars, Earth Magnetosphere, Emission Spectra, Stellar Luminosity, Stellar Radiation, Stellar Rotation, X Ray Sources

Scientific paper

It is proposed that the 1.24 sec pulses originate from luminosity variations at the source arising from time-varying accretion rather than from the passage of a beam of constant intensity past the earth. It is pointed out that the new model does not depend on any particular emission mechanism or beam width, puts no restriction on the angle between the rotation axis and the line-of-sight, and takes cognizance of the anisotropic distribution of accreting matter around the magnetosphere.

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