11 citations · 32 across the 9 of their papers we have counts for
9 papers
Concepts of inertial, gravitational and elementary particle masses
S. O. Tagieva, M. Erturk
In this article the concept of mass is analyzed based on the special and general relativity theories and particle (quantum) physics. The mass of a particle (m=E(0)/c^2) is determin…
Magnetospheric particle acceleration and X-ray emission of pulsars
Sevinc O. Tagieva, Askin Ankay, Arzu M. Ankay
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 fi…
The Strong Magnetic Field Decay and Evolution of Radio Pulsars on the P--P Diagram
O. H. Guseinov, A. Ankay, S. O. Tagieva
In this work we have analysed various data on radio pulsars and we have shown that magnetic field decay of a factor about 10-20 is necessary to explain their evolution, in particul…
Origin of PSRs with 0.1 < P < 0.3 s and 5 x 1E5 < Tau < 1E7 yr after the second Supernova explosion in HMXBs
O. H. Guseinov, A. O. Allakhverdiev, S. Tagieva +1
The origin of a part of the single pulsars with relatively low magnetic fields B < 1E12 G and with characteristic times Tau < 1E7 yr is established. Such pulsars occur as a result…
Dependences of the X-ray luminosity and pulsar wind nebula on different parameters of pulsars and the evolutionary effects
O. H. Guseinov, A. Ankay, S. O. Tagieva +1
Dependences of the X-ray luminosity (L) of single pulsars, due to ejection of relativistic particles, on electric field intensity, rate of rotational energy loss (Ė), magnetic…
The Lower Limit for Masses of Progenitors of Supernova Remnants and Radio Pulsars
Sevinc O. Tagieva, Oktay H. Guseinov, Askin Ankay
We examined correlations between young radio pulsars (PSRs), Supernova remnants (SNRs) which have different surface brightness values and young star formation regions (SFRs). Angul…