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Takayuki Yuasa978-4-431-54219-32013 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 €16210% OFF