Wave Zone Structure of NP 0532 and Infrared Radiation Excess of Crab Nebula
Abstract
At the distancer≳1015 cm from NP 0532 the plasma concentration decreases so that the intense low-frequency wave (ν=30 Hz) can propagate. The interaction of this wave with the electrons ejected from the pulsar should result in the IR radiation withFν∼102 fu at λ∼10 μ. This flux is the order of the excess IR radiation from the Crab Nebula.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- February 1975
- DOI:
- 10.1007/BF00643150
- Bibcode:
- 1975Ap&SS..32..375U
- Keywords:
-
- Astronomical Models;
- Crab Nebula;
- Infrared Radiation;
- Pulsars;
- Synchrotron Radiation;
- High Energy Electrons;
- Plasma Density;
- Plasma Waves;
- Plasma-Particle Interactions;
- Radiant Flux Density;
- Astrophysics;
- Radiation;
- Plasma Concentration;
- Infrared Radiation;
- Zone Structure;
- Wave Zone