Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-02-21
Astronomy and Astrophysics
Astrophysics
minor correction on table format, 20 pages (4 figures, 1 table), submitted to International Journal of Modern Physics D
Scientific paper
10.1142/S021827180801390X
The available data on isolated X-ray pulsars, their wind nebulae, and the supernova remnants which are connected to some of these sources are analyzed. It is shown that electric fields of neutron stars tear off charged particles from the surface of neutron star and trigger the acceleration of particles. The charged particles are accelerated mainly in the field of magneto-dipole radiation wave. Power and energy spectra of the charged particles depend on the strength of the magneto-dipole radiation. Therefore, the X-ray radiation is strongly dependent on the rate of rotational energy loss and weakly dependent on the electric field intensity. Coulomb interaction between the charged particles is the main factor for the energy loss and the X-ray spectra of the charged particles.
Ankay Arzu M.
Ankay Askin
Tagieva Sevinc O.
No associations
LandOfFree
Magnetospheric particle acceleration and X-ray emission of pulsars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Magnetospheric particle acceleration and X-ray emission of pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetospheric particle acceleration and X-ray emission of pulsars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-83676