Astronomy and Astrophysics – Astronomy
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996stan.reptq....m&link_type=abstract
Technical Report, Stanford Univ. Stanford, CA United States Dept. of Physics
Astronomy and Astrophysics
Astronomy
Black Holes (Astronomy), X Ray Astronomy, X Ray Binaries, Astronomical Observatories, Magnetic Fields, Binary Stars, Neutron Stars, Ginga Satellite
Scientific paper
The purpose of the research performed under N00014-93-2001 was to carry out analysis of x-ray temporal observations of several bright galactic x-ray binary systems containing neutron stars that are suspected to have weak magnetic fields and rapid spin periods and to study the X-ray timing signals from binaries suspected to contain black holes. Cygnus X-1 is such a source. The observations and analysis were done in a collaborative mode with the Naval Research Laboratory, Washington, D.C. and the Institute of Space and Astronautical Science (ISAS) of Japan. The observations were performed with the orbiting Japanese x-ray observatory Ginga. Analysis was done on computers at Stanford University, NRL and ISAS.
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