activity
20032022
most citedDistances of Galactic Radio Pulsars; First Quadrant: and

3 citations · 6 across the 4 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

5 papers · 2 filters

astro-ph2003

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…

astro-ph2003

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…

astro-ph2003

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…

astro-ph2003

Effects of the background radiation on radio pulsar and supernova remnant searches and the birth rates of these objects

Askin Ankay, Oktay H. Guseinov, Sevinc O. Tagieva

In different directions of the Galaxy the Galactic background radio radiation and radiation of complex star formation regions which include large number of OB associations have dif…

astro-ph2003

The Relation Between the Surface Brightness and the Diameter for Galactic Supernova Remnants

Oktay H. Guseinov, Askin Ankay, Aytap Sezer +1

In this work, we have constructed a relation between the surface brightness () and diameter (D) of Galactic C- and S-type supernova remnants (SNRs). In order to calibrate the $Σ…