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  • Shoji Kato
    978-4-431-56208-5
    2016
    Edition 1
    • Explains the current state of disk-oscillation theory, providing a potentially important tool to accurately determine spins of black hole sources in the universe
    • Clarifies our current understanding of discoseismology as it becomes more important in future in elucidating the structure and evolution of astrophysical disks
    • Describes quasi-periodic oscillations in X-ray binaries, superhumps in dwarf novae, and long-term variations in Be stars and Be/X-ray binaries
    €240 €216
    10% OFF

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