Results 11 to 20 of about 862,547 (224)
Almost 50 years after radio pulsars were discovered in 1967, our understanding of these objects remains incomplete. On the one hand, within a few years it became clear that neutron star rotation gives rise to the extremely stable sequence of radio pulses,
V. S. Beskin +3 more
semanticscholar +6 more sources
Magnetic fields of radio pulsars [PDF]
The mechanism of magnetodipole braking of radio pulsars is used to calculate new values of the surface magnetic fields of neutron stars. The angles β between the spin axes and magnetic moments of the neutron stars were estimated for 376 radio pulsars ...
E. B. Nikitina, I. Malov
semanticscholar +4 more sources
Timing of young radio pulsars – II. Braking indices and their interpretation [PDF]
In Paper I of this series, we detected a significant value of the braking index ($n$) for 19 young, high-$\dot{E}$ radio pulsars using $\sim$ 10 years of timing observations from the 64-m Parkes radio telescope.
A. Parthasarathy +14 more
semanticscholar +1 more source
Origin of Pulsar Radio Emission [PDF]
9 pages, 4 ...
Alexander Philippov +2 more
openaire +3 more sources
Braking indices of young radio pulsars: theoretical perspective [PDF]
Recently, Parthsarathy et al. analysed long-term timing observations of 85 young radio pulsars. They found that 11 objects have braking indices ranging $\sim 10-100$, far from the classical value $n=3$. They also noted a mild correlation between measured
A. Igoshev, S. Popov
semanticscholar +1 more source
RADIO EFFICIENCY OF PULSARS [PDF]
10 pages, 8 figures, 1 table, accepted for publication in ...
Szary, Andrzej +4 more
openaire +2 more sources
On the nature of pulsar radio emission [PDF]
39 pages, 10 ...
Lyutikov, Maxim +2 more
openaire +5 more sources
On the galactic distributions of radio pulsars and plasma density [PDF]
A brief review of distance measurement methods for some astronomical sources is presented. Galactic plasma density distribution as related to the distribution of radio pulsars is discussed and a method for constructing relations between ...
Ankay A., Yazgan E., Kutukcu P.
doaj +1 more source
Preprint of a chapter of the book 'Millisecond Pulsars', of the Astrophysics and Space Science Library (ASSL) series edited by Sudip Bhattacharyya, Alessandro Papitto and Dipankar Bhattacharya; 33 pages, 14 Figures, 3 ...
Bhattacharyya, Bhaswati, Roy, Jayanta
openaire +2 more sources
Radio Pulsars Resonantly Accelerating Electrons
Based on the recently demonstrated resonant wave–wave process, it is shown that electrons can be accelerated to ultra-relativistic energies in the magnetospheres of radio pulsars. The energization occurs via the resonant interaction of the electron wave (
Zaza N. Osmanov, Swadesh M. Mahajan
doaj +1 more source

