Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..271d&link_type=abstract
Astrophysics and Space Science, Volume 161, Issue 2, pp.271-278
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
In the magnetic axial ambience of the rapidly rotating pulsar, the position beam has been accelerated by the gap of the intense electric field, and ejected with rotation around the magnetic axis. While there exists rare plasma envelope near the pulsar, such energetic and rotational positron beam may have those waves near the ion-cyclotron frequencies amplified in the direction of the magnetic field, by exciting Čerenkov and maser instabilities. These are a kind of coherence radiation which has a larger portion of circular polarization. Under this mechanism, the emerging of another radiation process from the pulsars, that is, the core emission can be satisfactorily explained. This paper also discusses some possible observations resulting from the mechanism.
Deyu Wang
Hao Chen
Xinji Wu
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