Published April 7, 1975 | Version v1
Journal article Metadata-only

Synchrotron emission from an oblique rotator and its application to pulsars

Creators

  • 1. Division of Controlled Thermonuclear Research, U.S. Atomic Energy Commission, Washington, D.C. 20545

Description

A method is presented which permits rapid interpretation of the synchrotron patterns emitted by a charged particle moving in the uniform magnetic field of an oblique rotator. The analysis predicts a variety of intensity and polarization patterns that are compared with data from a number of pulsars. It also predicts the observed frequency dependence of the peak-to-peak separation of two double-peaked pulsars

Additional details

Identifiers

DOI
10.1103/physrevlett.34.901;

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
34
Journal Issue
14
Series
Phys. Rev. Lett.
Journal Page Range
901-905
ISSN
0031-9007

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
6203019
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHARGED PARTICLES; FREQUENCY DEPENDENCE; MAGNETIC FIELDS; POLARIZATION; POWER; PULSARS; ROTATION; SYNCHROTRON RADIATION
Descriptors DEC
BREMSSTRAHLUNG; COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS

Optional Information

Notes
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