Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://xray.sai.msu.ru/~mystery/articles/review/node20.html
Дата изменения: Tue Feb 25 19:24:12 1997 Дата индексирования: Tue Oct 2 14:40:25 2012 Кодировка: Поисковые слова: ngc 5128 |
Next: The
Corotation Radius Up: ``Ecology''
of Magnetic Rotators Previous: The
Stopping Radius in
Apparently, the magnetic field of a star becomes significant only when the stopping radius exceeds the radius of the star, . We take the Alfven radius for , since it is the smallest of the two quantities and . Hence, we can estimate the lowest value of magnetic field of a star which will influence the flow of matter
The case , is considered most frequently, and for this case we get the following numerical estimations
or, equivalently,
Most presently observed NS have magnetic fields G and dipole moments G cm , so the magnetic field must necessarily be taken into account when considering interaction of matter with these stars.