Drift model and the nature of AXPs and SGRs

Details Drift model and the nature of AXPs and SGRs Drift model and the nature of AXPs and SGRs

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..195m&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 195-196

Other

X-Ray Sources (Astronomical), Neutron Stars, Gamma-Rays, Magnetic Fields, X-Ray Sources, X-Ray Bursts, Neutron Stars, Gamma-Ray, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

Several models have been proposed for the description of anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs). The most widely discussed is the magnetar model, which involves a neutron stars with a surface magnetic field of the order of 1014÷1015 G [1]. Some other models put forward to explain the observed peculiarities of AXPs and SGRs. There is currently no model that can satisfactorily describe all the observational properties of these objects. We develope the drift model. Here, we discuss the applicability of the magnetar model and consider the feasibility of the drift model.

Affiliated with

Also associated with

No associations

Rating

Drift model and the nature of AXPs and SGRs 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 Drift model and the nature of AXPs and SGRs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Drift model and the nature of AXPs and SGRs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1738463