Zobrazeno 1 - 3
of 3
pro vyhledávání: '"O. V. Chedia"'
Publikováno v:
The Astrophysical Journal. 479:313-317
A new mechanism of wisp formation in the Crab Nebula, without recourse to a shock wave, is presented. The mechanism is based on the plasma processes taking place in the relativistic electron-positron plasma, in particular, on excitation of the drift
Publikováno v:
Scopus-Elsevier
An investigation of the kinematics of a rotating relativistic plasma stream in the perpendicular rotator model of the pulsar magnetosphere is presented. It is assumed that the plasma (ejected from the pulsar) moves along the pulsar magnetic field lin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7121f7f234971cb5056e3dbb2dd1070
http://arxiv.org/abs/astro-ph/9711265
http://arxiv.org/abs/astro-ph/9711265
Publikováno v:
Astrophysics and Space Science. 149:255-272
The mechanism of the large-scale magnetic field generation in the Crab Nebula is proposed. The basis for the considered ‘fast’ mechanism is the model of the central region of Crab Nebula amorphous part having the form of slightly divergent double