Published May 1977 | Version v1
Journal article

Model for the microstructure emission of pulsars

Creators

  • 1. Cambridge Univ. (UK). Observatories

Description

Recent observations of radio radiation have been used to construct a qualitative model of the emitting region near pulsars. The data can be reconciled with the view that dense regions, themselves containing many coherent radiating filaments, extend for long distances along the dipolar field lines. (author)

Additional details

Identifiers

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
179
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
311-315
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
8326599
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COHERENT RADIATION; PULSARS; RADIOWAVE RADIATION; STAR MODELS; WAVE PROPAGATION
Descriptors DEC
COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; MATHEMATICAL MODELS; RADIATIONS

Optional Information

Notes
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