Published 1984 | Version v1
Book Metadata-only

Model of radio emission of the millisecond pulsar PSR 1937+214

Creators

  • 1. National Radio Astronomy Observatory, Charlottesville, VA

Description

A model of radio emission of millisecond pulsar PSR 1937+214 is proposed. The emission region is expected to lie very close to the polar cap surface, where the contribution of the quadrupole component to the actual magnetic field may be significant. It is argued that the interpulse as well as the main pulse are emitted from the same magnetic pole. 9 references

Additional details

Publishing Information

Publisher
National Radio Astronomy Observatory.
Imprint Place
Green Bank, WV (USA)
Imprint Title
Birth and evolution of neutron stars: issues raised by millisecond pulsars
Journal Page Range
p. 146-150.

Conference

Title
Workshop on the millisecond pulsar.
Dates
6-8 Jun 1984.
Place
Green Bank, WV (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17080656
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
MAGNETIC FIELDS; MATHEMATICAL MODELS; NEUTRON STARS; PULSARS; PULSES; RADIOWAVE RADIATION; RELATIVISTIC RANGE
Descriptors DEC
COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; ENERGY RANGE; RADIATIONS; STARS