31 citations · 72 across the 13 of their papers we have counts for
13 papers
Acceleration of particles in pulsar magnetosphere and the X-ray radiation
Oktay H. Guseinov, Askin Ankay, Sevinc O. Tagieva
The available data of single X-ray pulsars, their wind nebulae, and the SNRs which are connected to some of these sources are analysed. It is shown that electric field intensity of…
Influences of neutron star parameters on evolutions of different types of pulsar; evolutions of anomalous X-ray pulsars, soft gamma repeaters and dim isolated thermal neutron stars on the P-P diagram
Oktay H. Guseinov, Askin Ankay, Sevinc O. Tagieva
Influences of the mass, moment of inertia, rotation, absence of stability in the atmosphere and some other parameters of neutron stars on the evolution of pulsars are examined. It…
Birth rates of different types of neutron star and possible evolutions of these objects
Oktay H. Guseinov, Askin Ankay, Sevinc O. Tagieva
We estimate the spatial densities of different types of neutron star near the Sun. It is shown that the distances of dim isolated thermal neutron stars must be on average about 300…
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…