Understanding the effects of geometry and rotation on pulsar intensity profiles
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/406/2/1029/18711162/mnr0406-1029.pdf
Reference52 articles.
1. Microtexture in the pulsar radio emission zone
2. A relativistic model of pulsar polarization
3. General Theory of Coherent Curvature Radiation
4. General Radiation Formulae for a Relativistic Charged Particle Moving in Curved Magnetic Field Lines: The Synchrocurvature Radiation Mechanism
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1. The Frequency-dependent Behavior of Subpulse Drifting. I. Carousel Geometry and Emission Heights of PSR B0031–07;The Astrophysical Journal;2019-09-18
2. Determining the rotation direction in pulsars;Nature Communications;2019-07-19
3. On the Geometry of Curvature Radiation and Implications for Subpulse Drifting;The Astrophysical Journal;2019-01-07
4. The origin of the frequency-dependent behaviour of pulsar radio profiles;Monthly Notices of the Royal Astronomical Society;2014-11-28
5. THE ROLE OF ROTATION AND POLAR-CAP CURRENTS ON PULSAR RADIO EMISSION AND POLARIZATION;The Astrophysical Journal;2013-05-10
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