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  • Takayuki Yuasa
    978-4-431-54219-3
    2013
    Edition 1
    • Provides an X-ray spectral model that estimates white dwarf masses by fitting observed data from the Suzaku observatory
    • Reveals that the observed broadband spectra of the Galactic ridge X-ray emission can be explained by a sum of spectra of known types of X-ray stars
    • Nominated as an outstanding contribution by the University of Tokyo's Physics Department in 2011
    €180 €162
    10% OFF

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