The role of proton cyclotron emission near accreting magnetic neutron stars

Details The role of proton cyclotron emission near accreting magnetic neutron stars The role of proton cyclotron emission near accreting magnetic neutron stars

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982japa....3..413a&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 3, Dec. 1982, p. 413-418.

Astronomy and Astrophysics

Astrophysics

Cyclotron Radiation, Gamma Ray Bursts, Magnetic Stars, Neutron Stars, X Ray Sources, Binary Stars, Protons, Stellar Mass Accretion

Scientific paper

The process of coherent and incoherent proton cyclotron emission occurring near the polar regions of a strongly magnetic accreting neutron star is considered. The soft X-ray flux resulting from the incoherent emission process is calculated for application to Her X-1 and also to gamma ray bursts, a consequence of which is that gamma ray bursts will be accompanied by soft X-ray bursts.

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