Physical conditions in the Crab Nebula

Автор: Bychkov K.V.
Журнал: ASTRONOMICHESKII ZHURNAL
Том: 51
Год издания: 1974
Первая страница: 712
Последняя страница: 720
Аннотация: The paper deals with the further development of Bychkov's (1973) two-component model of the Crab nebula, according to which the nebula contains a multitude of long narrow strong- and weak-field regions. The strong-field regions are as old as the nebula itself; they radiate at radio frequencies. The weak-field regions are periodically generated by the pulsar; they produce a synchrotron emission in the optical and X-ray range. It is shown that in the IR and millimeter wave spectrum of the nebula, there must exist a singularity, since the high and low-frequency emissions derive from regions of different nature. On the basis of the parallelism of the X-ray spectra of the nebula and pulsar, it is shown that the mechanism of electron acceleration in the 'cavern' between the nebula and pulsar does not affect the particle spectrum
Добавил в систему: Бычков Константин Вениаминович

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