Neutronensterne als Quellen kosmischer Röntgenstrahlung

Details Neutronensterne als Quellen kosmischer Röntgenstrahlung Neutronensterne als Quellen kosmischer Röntgenstrahlung

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979nw.....66..286t&link_type=abstract

Naturwissenschaften, Volume 66, Issue 6, pp.286-293

Physics

Scientific paper

Unlike single neutron stars which appear as radio pulsars, neutron stars in close binary systems emit intense X-radiation. These superdense objects are of interest not only as the end stages of stellar evolution but also as physical laboratories which are dominated by superstrong gravitational and magnetic fields and in which matter densities and temperatures attain extreme values.

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