Investigation of High-Mass X-ray binaries
X-ray astronomy, as a branch of astronomy, concentrates on the emission of X-ray of celestial bodies characterized by wavelengths ranging from 0.001 to 100 Å. The first X-ray satellites which have significantly contributed to the development of X-ray astronomy are: Uhuru, Einstein, Röntgensatellit (ROSAT), Advanced Satellite for Cosmology and Astrophysics (ASCA), Rossi X-ray Timing Explorer (RXTE), BeppoSAX, Chandra, and X-ray Multi-Mirror-Newton (XXM-Newton). Generally, an X-ray binary is the brightest source of X-ray emission in the universe, which is composed of a compact star (such as a white dwarf, neutron star, or black hole) and component star (a brown dwarf or white dwarf).
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