Published 1984 | Version v1
Book Metadata-only

Thermal origin of neutron star magnetic fields

Creators

  • 1. California Institute of Technology, Pasadena

Description

Mechanisms by which magnetic fields can be generated on neutron stars are discussed. Applications to ordinary radio pulsars, millisecond pulsars, and rapidly spinning pulsars in plerionic supernova remnants are discussed. 5 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. 205-212.

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
17080639
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
AGE ESTIMATION; COSMIC X-RAY SOURCES; MAGNETIC FIELDS; MORPHOLOGICAL CHANGES; NEUTRON STARS; ORIGIN; PULSARS; RADIOWAVE RADIATION; ROTATION; SUPERNOVA REMNANTS
Descriptors DEC
COSMIC RADIO SOURCES; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS; STARS