Magnetic field energy as a source of the radio luminosity of quasars View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2011-12

AUTHORS

D. M. Sedrakian, M. V. Hayrapetyan, N. S. Ayvazyan

ABSTRACT

Energy release in the superconducting core of a neutron star as neutron vortices move toward the boundary of the star’s core and crust is examined. It is shown that the rate of energy release is on the order of 1026-1030 erg/s, or sufficient to provide the radio luminosity of known pulsars. The energy release rates calculated under the assumption of asymmetric energy release are compared with observational data on the radio luminosity of 575 pulsars. More... »

PAGES

507-514

References to SciGraph publications

  • 1995-06. The models for radio emission from pulsars–The outstanding issues in JOURNAL OF ASTROPHYSICS AND ASTRONOMY
  • Journal

    TITLE

    Astrophysics

    ISSUE

    4

    VOLUME

    54

    Author Affiliations

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10511-011-9201-x

    DOI

    http://dx.doi.org/10.1007/s10511-011-9201-x

    DIMENSIONS

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