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astro-ph2003★ 720 cited
GRB Formation Rates inferred from the Spectral Peak Energy - Luminosity Relation
D. Yonetoku, T. Murakami, T. Nakamura +3
We investigate the GRB formation rate based on the relation between the spectral peak energy () and the isotropic luminosity. The --luminosity relation covers the ene…
astro-ph2003★ 15 cited
Fine Structure of the Thermal and Non-Thermal X-Rays in the SN 1006 Shell
A. Bamba, R. Yamazaki, M. Ueno +1
The North Eastern shell of SN 1006 is the most probable acceleration site of high energy electrons (up to about 100 TeV) with the Fermi acceleration mechanism at the shock front. W…