The magnetospheres of baryon stars

Details The magnetospheres of baryon stars The magnetospheres of baryon stars

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976afz....12..339a&link_type=abstract

Astrofizika, vol. 12, May 1976, p. 339-349. In Russian.

Astronomy and Astrophysics

Astrophysics

6

Baryons, Magnetic Stars, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Stellar Magnetospheres, Astrophysics, Plasma Temperature, Resistance Heating, Stellar Radiation

Scientific paper

The physical conditions in the magnetospheres of several pulsars were investigated with particular attention given to the pulsar P 0531. Attention is given to energy storage, magnetospheric transparence, plasma temperature, and mechanisms for magnetospheric heating and energy transfer. It is concluded that for P 0531 the magnetospheric plasma is kept in a hot state due to Joule heating caused by drift currents. In the case of the other pulsars examined (P 2043 and P 1706), the initial region of the magnetosphere is heated by stellar radiation, while the remainder (the main part) is heated by drift currents.

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