Zobrazeno 1 - 10
of 73
pro vyhledávání: '"I. F. Malov"'
Autor:
Z V Ken’ko, I F Malov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:1826-1842
Distribution of angles β between magnetic moments and rotation axes for radio pulsars with periods in the interval 0.1 s < P < 2 s has been obtained. This distribution is rather wide with a mean value of 23°. For the bulk of pulsars, the inclinatio
Analysis of the Parameters of Radio Pulsars with Giant Pulses Using the Principal Component Analysis
Autor:
I. F. Malov, O. I. Malov
Publikováno v:
Astronomy Reports. 67:263-271
Autor:
I. F. Malov, O. I. Malov
Publikováno v:
Astronomy Reports. 67:181-193
Autor:
I. F. Malov
Publikováno v:
Astronomy Reports. 66:12-24
Autor:
I. F. Malov, H. P. Marozava
Publikováno v:
Astronomy Reports. 66:25-31
Autor:
I. F. Malov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:809-817
A comparative analysis of the properties of 60 pulsars located in supernova remnants (SNRs) was carried out. We found that (1) anomalous X-ray pulsars (AXPs) and soft gamma repeaters (SGRs) are characterized by longer periods and higher values of per
Autor:
I. F. Malov, H. P. Marozava
Publikováno v:
Astronomy Reports. 64:738-755
We have carried out a comparative analysis of the parameters of two samples of radio pulsars. The first of them is characterized by periods $$P > 2$$ s, the second one—by the surface magnetic fields $${{B}_{s}} > 4.4 \times $$ 1013 G. The purpose f
Autor:
I. F. Malov, M. Timirkeeva
Publikováno v:
Astrophysics and Space Science. 365
Two parameters such as magnetic fields near the light cylinder $B_{lc} $ and rates of rotational energy losses $\frac{dE}{dt} $ for 1795 radio pulsars without high energy emission (R), 52 radio loud gamma-ray pulsars ( $\gamma$ +R), 33 radio quiet ga
Autor:
A. A. Loginov, I. F. Malov
Publikováno v:
Bulletin of the Lebedev Physics Institute. 45:218-222
A mechanism of pulsar accumulation over the galaxy plane, caused by deceleration in the gravitational field and stopping at a certain distance of z from the plane is proposed. For pulsars with velocities close to the average observed velocity of abou
Autor:
I. F. Malov, Yu. A. Baurov
Publikováno v:
Physics & Astronomy International Journal. 1:205-208
Two models of gamma-ray bursts using the theory of byuons (TB) are considered. This theory describes a “life’ of special unobservable discrete objects from which the surrounding space and the world of ultimate particles are formed. Basic axioms a