Inverse mapping of polarized optical emission from pulsars: basic formulation and determination of emission altitude
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/417/1/730/3033993/mnras0417-0730.pdf
Reference28 articles.
1. A Population of Gamma-Ray Millisecond Pulsars Seen with the Fermi Large Area Telescope
2. THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
3. Pair formation above pulsar polar caps - Structure of the low altitude acceleration zone
4. Energetic radiation from rapidly spinning pulsars. I - Outer magnetosphere gaps. II - VELA and Crab
5. Two‐Pole Caustic Model for High‐Energy Light Curves of Pulsars
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1. The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars;New Astronomy Reviews;2020-12
2. VLT polarimetry observations of the middle-aged pulsar PSR B0656+14;Astronomy & Astrophysics;2015-11
3. Circular polarization of synchrotron radiation in high magnetic fields;Monthly Notices of the Royal Astronomical Society;2015-04
4. HST optical polarimetry of the Vela pulsar and nebula;Monthly Notices of the Royal Astronomical Society;2014-09-30
5. The Galway astronomical Stokes polarimeter: an all-Stokes optical polarimeter with ultra-high time resolution;Experimental Astronomy;2013-06-28
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