Interpulse radio emission of pulsars

Details Interpulse radio emission of pulsars Interpulse radio emission of pulsars

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..117s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 117-130. In Russian.

Astronomy and Astrophysics

Astronomy

6

Pulsars, Pulsed Radiation, Radio Emission, Stellar Radiation, Electron Plasma, Plasma Generators, Pulsar Magnetospheres

Scientific paper

For 9 pulsars out of 39 observed pulse emission (⪆3 σ) is detected, unequally distributed in longitude and containing from 2 to 19% of the main pulse energy. This emission has a steeper spectrum than the main pulse emission in the 100 - 400 MHz range and comes from the pulsar's magnetosphere. A correlation is shown to exist between the relative energy of the interpulse emission and the magnetospheric parameters in the region of generation of electron-positron plasma. For 3 pulsars, the interpulse parameters have been determined, and in PSR 0919+16 a pulsed feature has been detected, preceding the main pulse by 65°.

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