Expected characteristics of pulsar gamma-ray radiation and the problem of its location

Details Expected characteristics of pulsar gamma-ray radiation and the problem of its location Expected characteristics of pulsar gamma-ray radiation and the problem of its location

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....96...36h&link_type=abstract

Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 36-51.

Astronomy and Astrophysics

Astronomy

5

Gamma Ray Astronomy, Gamma Ray Spectra, Pulsar Magnetospheres, Pulsars, Secondary Emission, Electron Acceleration, Mathematical Models, Radiative Transfer, Spectrum Analysis

Scientific paper

The transfer of gamma rays in the near pulsar magnetosphere of a parallel rotator is studied, with emphasis placed on determining the parameters characterizing the emitted spectrum, namely high energy cutoff, spectral slopes, and the energy range of secondary emission. A systematic and analytical investigation is made of their relaxation to the electron acceleration. It is shown that there exists a maximum pulsar period above which pair creation in the vicinity of the crust is impossible, whatever the electron acceleration conditions may be

Affiliated with

Also associated with

No associations

Rating

Expected characteristics of pulsar gamma-ray radiation and the problem of its location does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Expected characteristics of pulsar gamma-ray radiation and the problem of its location, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Expected characteristics of pulsar gamma-ray radiation and the problem of its location will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1785516