GINGA Studies of Black Hole Candidates: Multiwavelength Studies Using Temporal Lags and Coherence Function Analysis and GINGA Archival Studies of QPOs in LMXB Z-Sources

Mathematics – Functional Analysis

Scientific paper

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Neutron Stars, X Ray Binaries, Stellar Magnetic Fields, Black Holes (Astronomy), Spaceborne Astronomy, Time Signals, Functional Analysis, Accretion Disks, Gravitational Fields, Magnetic Moments, Galactic Cosmic Rays, Angular Momentum, Oscillations, Momentum Transfer, Stellar Rotation, Astronomical Models

Scientific paper

The purpose of the research 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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