Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-08-21
Int.J.Mod.Phys.D13:197-214,2004
Astronomy and Astrophysics
Astrophysics
revised version
Scientific paper
10.1142/S0218271804004505
Dependences of the X-ray luminosity (L$_x$) of single pulsars, due to ejection of relativistic particles, on electric field intensity, rate of rotational energy loss (\.{E}), magnetic field, period, and the energy spectra of the ejected particles are discussed. Influence of the magnetic field and effects of some other parameters of neutron stars on the L$_x$-\.{E} and the L$_x$-$\tau$ (characteristic time) dependences are considered. Evolutionary factors also play an important role in our considerations. We find that only the pulsars with L$_{2-10keV}$$>10^{33}$ erg/s have pulsar wind nebula around them. The pulsars from which $\gamma$-ray radiation has been observed have low X-ray luminosities in general.
Ankay Askin
Guseinov Oktay H.
Tagieva Sevinc O.
Taskin M. O.
No associations
LandOfFree
Dependences of the X-ray luminosity and pulsar wind nebula on different parameters of pulsars and the evolutionary effects 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 Dependences of the X-ray luminosity and pulsar wind nebula on different parameters of pulsars and the evolutionary effects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dependences of the X-ray luminosity and pulsar wind nebula on different parameters of pulsars and the evolutionary effects will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-542295