A model for explanation of GeV gamma-rays from the Crab Nebula as a result of inverse Compton radiation of the unshocked pulsar wind [0.03%]
一种解释蟹状星云GeV伽马射线的模型,该模型认为这些伽马射线源自未受激波影响的脉冲星风的逆康普顿辐射。
F.A. Aharonian; S.V. Bogovalov
F.A. Aharonian; S.V. Bogovalov
W. Schmidt; S.K. Solanki; B.W. Lites; A.M. Title; V. Martińez Pillet
W. Schmidt; S.K. Solanki; B.W. Lites; A.M. Title; V. Martińez Pillet
C.M. Boily; L. Detemple; N.T. Faber
C.M. Boily; L. Detemple; N.T. Faber