Wave zone structure of NP 0532 and infrared radiation excess of Crab Nebula

Details Wave zone structure of NP 0532 and infrared radiation excess of Crab Nebula Wave zone structure of NP 0532 and infrared radiation excess of Crab Nebula

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..32..375u&link_type=abstract

Astrophysics and Space Science, vol. 32, Feb. 1975, p. 375-377.

Astronomy and Astrophysics

Astrophysics

22

Astronomical Models, Crab Nebula, Infrared Radiation, Pulsars, Synchrotron Radiation, High Energy Electrons, Plasma Density, Plasma Waves, Plasma-Particle Interactions, Radiant Flux Density

Scientific paper

At the distance r ~ io'~ cm from NP 0532 the plasma concentration
decreases so that the intense low-frequency wave (v =30 Hz) can
propagate. The interaction of this wave with the electrons ejected from
the pulsar should result in the IR radiation with F~ 102 fu at )~ 10 p.
This flux is the order of the excess JR radiation from the Crab Nebula

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