Two-Component Model for the Interstellar Scattering along the Line of Sight to the Pulsar PSR B0136+57

Details Two-Component Model for the Interstellar Scattering along the Line of Sight to the Pulsar PSR B0136+57 Two-Component Model for the Interstellar Scattering along the Line of Sight to the Pulsar PSR B0136+57

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009chphl..26l9701z&link_type=abstract

Chinese Physics Letters, Volume 26, Issue 12, pp. 129701 (2009).

Physics

Scientific paper

A rigorous treatment of the refractive scintillation caused by a two-component interstellar scattering medium and a Kolmogorov form of density spectrum is discussed. It is assumed that the interstellar scattering medium is composed of a thin screen ISM and an extended interstellar medium. We conclude that the refractive scintillation caused by this two-component ISM scattering gives a more satisfactory explanation for the observed flux density variation than the single extended medium model along the line of sight to the pulsar PSR B0136+57.

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