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Proceedings of 8th INTEGRAL Workshop "The Restless Gamma-ray Universe" — PoS(INTEGRAL 2010)
Public data of different types of High Mass X-Ray Binaries have been analyzed. We have developed a classification scheme based on their temporal variability and spectral properties. We find that the Be X-Ray binaries tend to show harder spectra than those of Supergiant X-ray Binaries and that the use of the statistical normalized variance seems to be a promising tool to identify source type.doi:10.22323/1.115.0119 fatcat:l6rbaz5qmjhw3frrovrzrxubee